*AI Summary*
A suitable group to review this material would be *Senior Aerospace Safety Engineers and Life Support Systems (LSS) Specialists.* These professionals are responsible for risk mitigation, atmospheric management, and emergency protocol development for crewed spaceflight.
### *Abstract*
This technical overview examines the unique physics, historical precedents, and mitigation strategies regarding fire in microgravity environments. Unlike Earth-based combustion, which is driven by buoyancy and convection, microgravity fire is governed by molecular diffusion, resulting in spherical, cooler, and slower-burning flames that can persist in low-oxygen environments. The analysis highlights that the primary threat to crew survival is not thermal damage but the rapid accumulation of toxic combustion byproducts—such as carbon monoxide, hydrogen cyanide, and hydrogen fluoride—within a closed-loop atmospheric system.
The transcript details the 1997 Mir oxygen generator fire as a critical case study in self-oxidizing "torch" fires and reviews the evolution of suppression technology from hazardous Halon systems to modern CO2 and fine-water-mist extinguishers used on the International Space Station (ISS). Finally, it emphasizes that 99% of spaceflight fire safety resides in prevention through rigorous materials testing and the elimination of ignition sources.
---
### *Aerospace Safety Analysis: Fire Dynamics and Suppression in Microgravity*
* *0:01:20 Combustion Physics in Microgravity:* In the absence of gravity, buoyancy-driven convection is eliminated. Flames form spherical shapes where oxygen reaches the fuel only via diffusion. These flames burn slower and cooler but can be sustained at lower oxygen concentrations than those on Earth.
* *0:02:50 NASA Combustion Research:* Experiments such as Flex 2, Acme, and Sophie utilize the Combustion Integrated Rack (CIR) on the ISS to study "cool flames" and flame propagation across materials. The Sapphire experiments conduct larger-scale burns on departing cargo vessels to safely observe fire behavior in pressurized volumes.
* *0:04:34 Atmospheric Contamination Risks:* The primary hazard in spacecraft fires is the contamination of the breathable atmosphere. Incomplete combustion produces high levels of soot and neurotoxins like carbon monoxide (CO) and hydrogen cyanide (HCN), as well as acidic vapors (HCl, HF) from burning polymers.
* *0:08:33 The 1997 Mir SFOG Incident:* A solid-fuel oxygen generator (lithium perchlorate) failed, likely due to a latex contaminant, creating a 3-foot-long torch-like jet of flame. The fire was self-oxidizing, making it immune to oxygen-starvation tactics and causing significant structural scorching and smoke.
* *0:11:41 Suppression Tactics on Mir:* Crew members used water-based extinguishers to cool the flame. A critical technical takeaway was the necessity of crew bracing; the thrust from the extinguisher pushed the operator backward in the weightless environment.
* *0:14:11 Historical Soviet Fire Records:* Previous incidents on Salyut 1 (electrical fire) and Salyut 6 (control panel fire) underscored the necessity of isolating power and fans to stop air circulation from feeding a fire.
* *0:15:33 Evolution of NASA Suppression Systems:*
* *Apollo:* Developed a nitrogen/freon foam (untested in actual flight).
* *Space Shuttle:* Utilized Halon 1301. While effective, its toxic byproducts required an immediate emergency landing if deployed.
* *ISS:* Employs CO2 extinguishers (compatible with CO2 scrubbers) and modern Water Mist extinguishers.
* *0:19:41 Water Mist Suppression:* Fine-mist systems create micron-sized droplets that maximize surface area for heat absorption and oxygen displacement without forming large, hazardous liquid globules.
* *0:20:21 Lithium-Ion Thermal Runaway:* Modern electronics present a risk of internal chemical fires. While extinguishers cannot stop the internal reaction, water mist is used to cool the surrounding environment and absorb evolved toxins.
* *0:22:37 Materials Prevention Protocols:* 99% of safety is achieved through material selection. Standards include using fire-retardant hook-and-loop fasteners (Velcro), limiting patch sizes to four square inches, and replacing flammable polyethylene trash bags with Armor Flex 301.
* *0:24:34 Future Mission Considerations:* Exploration of the Moon, Mars, and Titan will require safety systems adaptable to both partial gravity and microgravity, as smoke detection and flame propagation vary significantly with gravitational shifts.
AI-generated summary created with gemini-3-flash-preview for free via RocketRecap-dot-com. (Input: 22,375 tokens, Output: 967 tokens, Est. cost: $0.0141).Below, I will provide input for an example video (comprising of title, description, and transcript, in this order) and the corresponding abstract and summary I expect. Afterward, I will provide a new transcript that I want a summarization in the same format.
**Please give an abstract of the transcript and then summarize the transcript in a self-contained bullet list format.** Include starting timestamps, important details and key takeaways.
Example Input:
Fluidigm Polaris Part 2- illuminator and camera
mikeselectricstuff
131K subscribers
Subscribed
369
Share
Download
Clip
Save
5,857 views Aug 26, 2024
Fluidigm Polaris part 1 : • Fluidigm Polaris (Part 1) - Biotech g...
Ebay listings: https://www.ebay.co.uk/usr/mikeselect...
Merch https://mikeselectricstuff.creator-sp...
Transcript
Follow along using the transcript.
Show transcript
mikeselectricstuff
131K subscribers
Videos
About
Support on Patreon
40 Comments
@robertwatsonbath
6 hours ago
Thanks Mike. Ooof! - with the level of bodgery going on around 15:48 I think shame would have made me do a board re spin, out of my own pocket if I had to.
1
Reply
@Muonium1
9 hours ago
The green LED looks different from the others and uses phosphor conversion because of the "green gap" problem where green InGaN emitters suffer efficiency droop at high currents. Phosphide based emitters don't start becoming efficient until around 600nm so also can't be used for high power green emitters. See the paper and plot by Matthias Auf der Maur in his 2015 paper on alloy fluctuations in InGaN as the cause of reduced external quantum efficiency at longer (green) wavelengths.
4
Reply
1 reply
@tafsirnahian669
10 hours ago (edited)
Can this be used as an astrophotography camera?
Reply
mikeselectricstuff
·
1 reply
@mikeselectricstuff
6 hours ago
Yes, but may need a shutter to avoid light during readout
Reply
@2010craggy
11 hours ago
Narrowband filters we use in Astronomy (Astrophotography) are sided- they work best passing light in one direction so I guess the arrows on the filter frames indicate which way round to install them in the filter wheel.
1
Reply
@vitukz
12 hours ago
A mate with Channel @extractions&ire could use it
2
Reply
@RobertGallop
19 hours ago
That LED module says it can go up to 28 amps!!! 21 amps for 100%. You should see what it does at 20 amps!
Reply
@Prophes0r
19 hours ago
I had an "Oh SHIT!" moment when I realized that the weird trapezoidal shape of that light guide was for keystone correction of the light source.
Very clever.
6
Reply
@OneBiOzZ
20 hours ago
given the cost of the CCD you think they could have run another PCB for it
9
Reply
@tekvax01
21 hours ago
$20 thousand dollars per minute of run time!
1
Reply
@tekvax01
22 hours ago
"We spared no expense!" John Hammond Jurassic Park.
*(that's why this thing costs the same as a 50-seat Greyhound Bus coach!)
Reply
@florianf4257
22 hours ago
The smearing on the image could be due to the fact that you don't use a shutter, so you see brighter stripes under bright areas of the image as you still iluminate these pixels while the sensor data ist shifted out towards the top. I experienced this effect back at university with a LN-Cooled CCD for Spectroscopy. The stripes disapeared as soon as you used the shutter instead of disabling it in the open position (but fokussing at 100ms integration time and continuous readout with a focal plane shutter isn't much fun).
12
Reply
mikeselectricstuff
·
1 reply
@mikeselectricstuff
12 hours ago
I didn't think of that, but makes sense
2
Reply
@douro20
22 hours ago (edited)
The red LED reminds me of one from Roithner Lasertechnik. I have a Symbol 2D scanner which uses two very bright LEDs from that company, one red and one red-orange. The red-orange is behind a lens which focuses it into an extremely narrow beam.
1
Reply
@RicoElectrico
23 hours ago
PFG is Pulse Flush Gate according to the datasheet.
Reply
@dcallan812
23 hours ago
Very interesting. 2x
Reply
@littleboot_
1 day ago
Cool interesting device
Reply
@dav1dbone
1 day ago
I've stripped large projectors, looks similar, wonder if some of those castings are a magnesium alloy?
Reply
@kevywevvy8833
1 day ago
ironic that some of those Phlatlight modules are used in some of the cheapest disco lights.
1
Reply
1 reply
@bill6255
1 day ago
Great vid - gets right into subject in title, its packed with information, wraps up quickly. Should get a YT award! imho
3
Reply
@JAKOB1977
1 day ago (edited)
The whole sensor module incl. a 5 grand 50mpix sensor for 49 £.. highest bid atm
Though also a limited CCD sensor, but for the right buyer its a steal at these relative low sums.
Architecture Full Frame CCD (Square Pixels)
Total Number of Pixels 8304 (H) × 6220 (V) = 51.6 Mp
Number of Effective Pixels 8208 (H) × 6164 (V) = 50.5 Mp
Number of Active Pixels 8176 (H) × 6132 (V) = 50.1 Mp
Pixel Size 6.0 m (H) × 6.0 m (V)
Active Image Size 49.1 mm (H) × 36.8 mm (V)
61.3 mm (Diagonal),
645 1.1x Optical Format
Aspect Ratio 4:3
Horizontal Outputs 4
Saturation Signal 40.3 ke−
Output Sensitivity 31 V/e−
Quantum Efficiency
KAF−50100−CAA
KAF−50100−AAA
KAF−50100−ABA (with Lens)
22%, 22%, 16% (Peak R, G, B)
25%
62%
Read Noise (f = 18 MHz) 12.5 e−
Dark Signal (T = 60°C) 42 pA/cm2
Dark Current Doubling Temperature 5.7°C
Dynamic Range (f = 18 MHz) 70.2 dB
Estimated Linear Dynamic Range
(f = 18 MHz)
69.3 dB
Charge Transfer Efficiency
Horizontal
Vertical
0.999995
0.999999
Blooming Protection
(4 ms Exposure Time)
800X Saturation Exposure
Maximum Date Rate 18 MHz
Package Ceramic PGA
Cover Glass MAR Coated, 2 Sides or
Clear Glass
Features
• TRUESENSE Transparent Gate Electrode
for High Sensitivity
• Ultra-High Resolution
• Board Dynamic Range
• Low Noise Architecture
• Large Active Imaging Area
Applications
• Digitization
• Mapping/Aerial
• Photography
• Scientific
Thx for the tear down Mike, always a joy
Reply
@martinalooksatthings
1 day ago
15:49 that is some great bodging on of caps, they really didn't want to respin that PCB huh
8
Reply
@RhythmGamer
1 day ago
Was depressed today and then a new mike video dropped and now I’m genuinely happy to get my tear down fix
1
Reply
@dine9093
1 day ago (edited)
Did you transfrom into Mr Blobby for a moment there?
2
Reply
@NickNorton
1 day ago
Thanks Mike. Your videos are always interesting.
5
Reply
@KeritechElectronics
1 day ago
Heavy optics indeed... Spare no expense, cost no object. Splendid build quality. The CCD is a thing of beauty!
1
Reply
@YSoreil
1 day ago
The pricing on that sensor is about right, I looked in to these many years ago when they were still in production since it's the only large sensor you could actually buy. Really cool to see one in the wild.
2
Reply
@snik2pl
1 day ago
That leds look like from led projector
Reply
@vincei4252
1 day ago
TDI = Time Domain Integration ?
1
Reply
@wolpumba4099
1 day ago (edited)
Maybe the camera should not be illuminated during readout.
From the datasheet of the sensor (Onsemi): saturation 40300 electrons, read noise 12.5 electrons per pixel @ 18MHz (quite bad). quantum efficiency 62% (if it has micro lenses), frame rate 1 Hz. lateral overflow drain to prevent blooming protects against 800x (factor increases linearly with exposure time) saturation exposure (32e6 electrons per pixel at 4ms exposure time), microlens has +/- 20 degree acceptance angle
i guess it would be good for astrophotography
4
Reply
@txm100
1 day ago (edited)
Babe wake up a new mikeselectricstuff has dropped!
9
Reply
@vincei4252
1 day ago
That looks like a finger-lakes filter wheel, however, for astronomy they'd never use such a large stepper.
1
Reply
@MRooodddvvv
1 day ago
yaaaaay ! more overcomplicated optical stuff !
4
Reply
1 reply
@NoPegs
1 day ago
He lives!
11
Reply
1 reply
Transcript
0:00
so I've stripped all the bits of the
0:01
optical system so basically we've got
0:03
the uh the camera
0:05
itself which is mounted on this uh very
0:09
complex
0:10
adjustment thing which obviously to set
0:13
you the various tilt and uh alignment
0:15
stuff then there's two of these massive
0:18
lenses I've taken one of these apart I
0:20
think there's something like about eight
0:22
or nine Optical elements in here these
0:25
don't seem to do a great deal in terms
0:26
of electr magnification they're obiously
0:28
just about getting the image to where it
0:29
uh where it needs to be just so that
0:33
goes like that then this Optical block I
0:36
originally thought this was made of some
0:37
s crazy heavy material but it's just
0:39
really the sum of all these Optical bits
0:41
are just ridiculously heavy those lenses
0:43
are about 4 kilos each and then there's
0:45
this very heavy very solid um piece that
0:47
goes in the middle and this is so this
0:49
is the filter wheel assembly with a
0:51
hilariously oversized steper
0:53
motor driving this wheel with these very
0:57
large narrow band filters so we've got
1:00
various different shades of uh
1:03
filters there five Al together that
1:06
one's actually just showing up a silver
1:07
that's actually a a red but fairly low
1:10
transmission orangey red blue green
1:15
there's an excess cover on this side so
1:16
the filters can be accessed and changed
1:19
without taking anything else apart even
1:21
this is like ridiculous it's like solid
1:23
aluminium this is just basically a cover
1:25
the actual wavelengths of these are um
1:27
488 525 570 630 and 700 NM not sure what
1:32
the suffix on that perhaps that's the uh
1:34
the width of the spectral line say these
1:37
are very narrow band filters most of
1:39
them are you very little light through
1:41
so it's still very tight narrow band to
1:43
match the um fluoresence of the dies
1:45
they're using in the biochemical process
1:48
and obviously to reject the light that's
1:49
being fired at it from that Illuminator
1:51
box and then there's a there's a second
1:53
one of these lenses then the actual sort
1:55
of samples below that so uh very serious
1:58
amount of very uh chunky heavy Optics
2:01
okay let's take a look at this light
2:02
source made by company Lumen Dynamics
2:04
who are now part of
2:06
excelitas self-contained unit power
2:08
connector USB and this which one of the
2:11
Cable Bundle said was a TTL interface
2:14
USB wasn't used in uh the fluid
2:17
application output here and I think this
2:19
is an input for um light feedback I
2:21
don't if it's regulated or just a measur
2:23
measurement facility and the uh fiber
2:27
assembly
2:29
Square Inlet there and then there's two
2:32
outputs which have uh lens assemblies
2:35
and this small one which goes back into
2:37
that small Port just Loops out of here
2:40
straight back in So on this side we've
2:42
got the electronics which look pretty
2:44
straightforward we've got a bit of power
2:45
supply stuff over here and we've got
2:48
separate drivers for each wavelength now
2:50
interesting this is clearly been very
2:52
specifically made for this application
2:54
you I was half expecting like say some
2:56
generic drivers that could be used for a
2:58
number of different things but actually
3:00
literally specified the exact wavelength
3:02
on the PCB there is provision here for
3:04
385 NM which isn't populated but this is
3:07
clearly been designed very specifically
3:09
so these four drivers look the same but
3:10
then there's two higher power ones for
3:12
575 and
3:14
520 a slightly bigger heat sink on this
3:16
575 section there a p 24 which is
3:20
providing USB interface USB isolator the
3:23
USB interface just presents as a comport
3:26
I did have a quick look but I didn't
3:27
actually get anything sensible um I did
3:29
dump the Pi code out and there's a few
3:31
you a few sort of commands that you
3:32
could see in text but I didn't actually
3:34
manage to get it working properly I
3:36
found some software for related version
3:38
but it didn't seem to want to talk to it
3:39
but um I say that wasn't used for the
3:41
original application it might be quite
3:42
interesting to get try and get the Run
3:44
hours count out of it and the TTL
3:46
interface looks fairly straightforward
3:48
we've got positions for six opto
3:50
isolators but only five five are
3:52
installed so that corresponds with the
3:54
unused thing so I think this hopefully
3:56
should be as simple as just providing a
3:57
ttrl signal for each color to uh enable
4:00
it a big heat sink here which is there I
4:03
think there's like a big S of metal
4:04
plate through the middle of this that
4:05
all the leads are mounted on the other
4:07
side so this is heat sinking it with a
4:09
air flow from a uh just a fan in here
4:13
obviously don't have the air flow
4:14
anywhere near the Optics so conduction
4:17
cool through to this plate that's then
4:18
uh air cooled got some pots which are
4:21
presumably power
4:22
adjustments okay let's take a look at
4:24
the other side which is uh much more
4:27
interesting see we've got some uh very
4:31
uh neatly Twisted cable assemblies there
4:35
a bunch of leads so we've got one here
4:37
475 up here 430 NM 630 575 and 520
4:44
filters and dcro mirrors a quick way to
4:48
see what's white is if we just shine
4:49
some white light through
4:51
here not sure how it is is to see on the
4:54
camera but shining white light we do
4:55
actually get a bit of red a bit of blue
4:57
some yellow here so the obstacle path
5:00
575 it goes sort of here bounces off
5:03
this mirror and goes out the 520 goes
5:07
sort of down here across here and up
5:09
there 630 goes basically straight
5:13
through
5:15
430 goes across there down there along
5:17
there and the 475 goes down here and
5:20
left this is the light sensing thing
5:22
think here there's just a um I think
5:24
there a photo diode or other sensor
5:26
haven't actually taken that off and
5:28
everything's fixed down to this chunk of
5:31
aluminium which acts as the heat
5:32
spreader that then conducts the heat to
5:33
the back side for the heat
5:35
sink and the actual lead packages all
5:38
look fairly similar except for this one
5:41
on the 575 which looks quite a bit more
5:44
substantial big spay
5:46
Terminals and the interface for this
5:48
turned out to be extremely simple it's
5:50
literally a 5V TTL level to enable each
5:54
color doesn't seem to be any tensity
5:56
control but there are some additional
5:58
pins on that connector that weren't used
5:59
in the through time thing so maybe
6:01
there's some extra lines that control
6:02
that I couldn't find any data on this uh
6:05
unit and the um their current product
6:07
range is quite significantly different
6:09
so we've got the uh blue these
6:13
might may well be saturating the camera
6:16
so they might look a bit weird so that's
6:17
the 430
6:18
blue the 575
6:24
yellow uh
6:26
475 light blue
6:29
the uh 520
6:31
green and the uh 630 red now one
6:36
interesting thing I noticed for the
6:39
575 it's actually it's actually using a
6:42
white lead and then filtering it rather
6:44
than using all the other ones are using
6:46
leads which are the fundamental colors
6:47
but uh this is actually doing white and
6:50
it's a combination of this filter and
6:52
the dichroic mirrors that are turning to
6:55
Yellow if we take the filter out and a
6:57
lot of the a lot of the um blue content
7:00
is going this way the red is going
7:02
straight through these two mirrors so
7:05
this is clearly not reflecting much of
7:08
that so we end up with the yellow coming
7:10
out of uh out of there which is a fairly
7:14
light yellow color which you don't
7:16
really see from high intensity leads so
7:19
that's clearly why they've used the
7:20
white to uh do this power consumption of
7:23
the white is pretty high so going up to
7:25
about 2 and 1 half amps on that color
7:27
whereas most of the other colors are
7:28
only drawing half an amp or so at 24
7:30
volts the uh the green is up to about
7:32
1.2 but say this thing is uh much
7:35
brighter and if you actually run all the
7:38
colors at the same time you get a fairly
7:41
reasonable um looking white coming out
7:43
of it and one thing you might just be
7:45
out to notice is there is some sort
7:46
color banding around here that's not
7:49
getting uh everything s completely
7:51
concentric and I think that's where this
7:53
fiber optic thing comes
7:58
in I'll
8:00
get a couple of Fairly accurately shaped
8:04
very sort of uniform color and looking
8:06
at What's um inside here we've basically
8:09
just got this Square Rod so this is
8:12
clearly yeah the lights just bouncing
8:13
off all the all the various sides to um
8:16
get a nice uniform illumination uh this
8:19
back bit looks like it's all potted so
8:21
nothing I really do to get in there I
8:24
think this is fiber so I have come
8:26
across um cables like this which are
8:27
liquid fill but just looking through the
8:30
end of this it's probably a bit hard to
8:31
see it does look like there fiber ends
8:34
going going on there and so there's this
8:36
feedback thing which is just obviously
8:39
compensating for the any light losses
8:41
through here to get an accurate
8:43
representation of uh the light that's
8:45
been launched out of these two
8:47
fibers and you see uh
8:49
these have got this sort of trapezium
8:54
shape light guides again it's like a
8:56
sort of acrylic or glass light guide
9:00
guess projected just to make the right
9:03
rectangular
9:04
shape and look at this Center assembly
9:07
um the light output doesn't uh change
9:10
whether you feed this in or not so it's
9:11
clear not doing any internal Clos Loop
9:14
control obviously there may well be some
9:16
facility for it to do that but it's not
9:17
being used in this
9:19
application and so this output just
9:21
produces a voltage on the uh outle
9:24
connector proportional to the amount of
9:26
light that's present so there's a little
9:28
diffuser in the back there
9:30
and then there's just some kind of uh
9:33
Optical sensor looks like a
9:35
chip looking at the lead it's a very
9:37
small package on the PCB with this lens
9:40
assembly over the top and these look
9:43
like they're actually on a copper
9:44
Metalized PCB for maximum thermal
9:47
performance and yeah it's a very small
9:49
package looks like it's a ceramic
9:51
package and there's a thermister there
9:53
for temperature monitoring this is the
9:56
475 blue one this is the 520 need to
9:59
Green which is uh rather different OB
10:02
it's a much bigger D with lots of bond
10:04
wise but also this looks like it's using
10:05
a phosphor if I shine a blue light at it
10:08
lights up green so this is actually a
10:10
phosphor conversion green lead which
10:12
I've I've come across before they want
10:15
that specific wavelength so they may be
10:17
easier to tune a phosphor than tune the
10:20
um semiconductor material to get the uh
10:23
right right wavelength from the lead
10:24
directly uh red 630 similar size to the
10:28
blue one or does seem to have a uh a
10:31
lens on top of it there is a sort of red
10:33
coloring to
10:35
the die but that doesn't appear to be
10:38
fluorescent as far as I can
10:39
tell and the white one again a little
10:41
bit different sort of much higher
10:43
current
10:46
connectors a makeer name on that
10:48
connector flot light not sure if that's
10:52
the connector or the lead
10:54
itself and obviously with the phosphor
10:56
and I'd imagine that phosphor may well
10:58
be tuned to get the maximum to the uh 5
11:01
cenm and actually this white one looks
11:04
like a St fairly standard product I just
11:06
found it in Mouse made by luminous
11:09
devices in fact actually I think all
11:11
these are based on various luminous
11:13
devices modules and they're you take
11:17
looks like they taking the nearest
11:18
wavelength and then just using these
11:19
filters to clean it up to get a precise
11:22
uh spectral line out of it so quite a
11:25
nice neat and um extreme
11:30
bright light source uh sure I've got any
11:33
particular use for it so I think this
11:35
might end up on
11:36
eBay but uh very pretty to look out and
11:40
without the uh risk of burning your eyes
11:43
out like you do with lasers so I thought
11:45
it would be interesting to try and
11:46
figure out the runtime of this things
11:48
like this we usually keep some sort
11:49
record of runtime cuz leads degrade over
11:51
time I couldn't get any software to work
11:52
through the USB face but then had a
11:54
thought probably going to be writing the
11:55
runtime periodically to the e s prom so
11:58
I just just scope up that and noticed it
12:00
was doing right every 5 minutes so I
12:02
just ran it for a while periodically
12:04
reading the E squ I just held the pick
12:05
in in reset and um put clip over to read
12:07
the square prom and found it was writing
12:10
one location per color every 5 minutes
12:12
so if one color was on it would write
12:14
that location every 5 minutes and just
12:16
increment it by one so after doing a few
12:18
tests with different colors of different
12:19
time periods it looked extremely
12:21
straightforward it's like a four bite
12:22
count for each color looking at the
12:24
original data that was in it all the
12:26
colors apart from Green were reading
12:28
zero and the green was reading four
12:30
indicating a total 20 minutes run time
12:32
ever if it was turned on run for a short
12:34
time then turned off that might not have
12:36
been counted but even so indicates this
12:37
thing wasn't used a great deal the whole
12:40
s process of doing a run can be several
12:42
hours but it'll only be doing probably
12:43
the Imaging at the end of that so you
12:46
wouldn't expect to be running for a long
12:47
time but say a single color for 20
12:50
minutes over its whole lifetime does
12:52
seem a little bit on the low side okay
12:55
let's look at the camera un fortunately
12:57
I managed to not record any sound when I
12:58
did this it's also a couple of months
13:00
ago so there's going to be a few details
13:02
that I've forgotten so I'm just going to
13:04
dub this over the original footage so um
13:07
take the lid off see this massive great
13:10
heat sink so this is a pel cool camera
13:12
we've got this blower fan producing a
13:14
fair amount of air flow through
13:16
it the connector here there's the ccds
13:19
mounted on the board on the
13:24
right this unplugs so we've got a bit of
13:27
power supply stuff on here
13:29
USB interface I think that's the Cyprus
13:32
microcontroller High speeded USB
13:34
interface there's a zyink spon fpga some
13:40
RAM and there's a couple of ATD
13:42
converters can't quite read what those
13:45
those are but anal
13:47
devices um little bit of bodgery around
13:51
here extra decoupling obviously they
13:53
have having some noise issues this is
13:55
around the ram chip quite a lot of extra
13:57
capacitors been added there
13:59
uh there's a couple of amplifiers prior
14:01
to the HD converter buffers or Andor
14:05
amplifiers taking the CCD
14:08
signal um bit more power spy stuff here
14:11
this is probably all to do with
14:12
generating the various CCD bias voltages
14:14
they uh need quite a lot of exotic
14:18
voltages next board down is just a
14:20
shield and an interconnect
14:24
boardly shielding the power supply stuff
14:26
from some the more sensitive an log
14:28
stuff
14:31
and this is the bottom board which is
14:32
just all power supply
14:34
stuff as you can see tons of capacitors
14:37
or Transformer in
14:42
there and this is the CCD which is a uh
14:47
very impressive thing this is a kf50 100
14:50
originally by true sense then codec
14:53
there ON
14:54
Semiconductor it's 50 megapixels uh the
14:58
only price I could find was this one
15:00
5,000 bucks and the architecture you can
15:03
see there actually two separate halves
15:04
which explains the Dual AZ converters
15:06
and two amplifiers it's literally split
15:08
down the middle and duplicated so it's
15:10
outputting two streams in parallel just
15:13
to keep the bandwidth sensible and it's
15:15
got this amazing um diffraction effects
15:18
it's got micro lenses over the pixel so
15:20
there's there's a bit more Optics going
15:22
on than on a normal
15:25
sensor few more bodges on the CCD board
15:28
including this wire which isn't really
15:29
tacked down very well which is a bit uh
15:32
bit of a mess quite a few bits around
15:34
this board where they've uh tacked
15:36
various bits on which is not super
15:38
impressive looks like CCD drivers on the
15:40
left with those 3 ohm um damping
15:43
resistors on the
15:47
output get a few more little bodges
15:50
around here some of
15:52
the and there's this separator the
15:54
silica gel to keep the moisture down but
15:56
there's this separator that actually
15:58
appears to be cut from piece of
15:59
antistatic
16:04
bag and this sort of thermal block on
16:06
top of this stack of three pel Cola
16:12
modules so as with any Stacks they get
16:16
um larger as they go back towards the
16:18
heat sink because each P's got to not
16:20
only take the heat from the previous but
16:21
also the waste heat which is quite
16:27
significant you see a little temperature
16:29
sensor here that copper block which
16:32
makes contact with the back of the
16:37
CCD and this's the back of the
16:40
pelas this then contacts the heat sink
16:44
on the uh rear there a few thermal pads
16:46
as well for some of the other power
16:47
components on this
16:51
PCB okay I've connected this uh camera
16:54
up I found some drivers on the disc that
16:56
seem to work under Windows 7 couldn't
16:58
get to install under Windows 11 though
17:01
um in the absence of any sort of lens or
17:03
being bothered to the proper amount I've
17:04
just put some f over it and put a little
17:06
pin in there to make a pinhole lens and
17:08
software gives a few options I'm not
17:11
entirely sure what all these are there's
17:12
obviously a clock frequency 22 MHz low
17:15
gain and with PFG no idea what that is
17:19
something something game programmable
17:20
Something game perhaps ver exposure
17:23
types I think focus is just like a
17:25
continuous grab until you tell it to
17:27
stop not entirely sure all these options
17:30
are obviously exposure time uh triggers
17:33
there ex external hardware trigger inut
17:35
you just trigger using a um thing on
17:37
screen so the resolution is 8176 by
17:40
6132 and you can actually bin those
17:42
where you combine multiple pixels to get
17:46
increased gain at the expense of lower
17:48
resolution down this is a 10sec exposure
17:51
obviously of the pin hole it's very uh
17:53
intensitive so we just stand still now
17:56
downloading it there's the uh exposure
17:59
so when it's
18:01
um there's a little status thing down
18:03
here so that tells you the um exposure
18:07
[Applause]
18:09
time it's this is just it
18:15
downloading um it is quite I'm seeing
18:18
quite a lot like smearing I think that I
18:20
don't know whether that's just due to
18:21
pixels overloading or something else I
18:24
mean yeah it's not it's not um out of
18:26
the question that there's something not
18:27
totally right about this camera
18:28
certainly was bodge wise on there um I
18:31
don't I'd imagine a camera like this
18:32
it's got a fairly narrow range of
18:34
intensities that it's happy with I'm not
18:36
going to spend a great deal of time on
18:38
this if you're interested in this camera
18:40
maybe for astronomy or something and
18:42
happy to sort of take the risk of it may
18:44
not be uh perfect I'll um I think I'll
18:47
stick this on eBay along with the
18:48
Illuminator I'll put a link down in the
18:50
description to the listing take your
18:52
chances to grab a bargain so for example
18:54
here we see this vertical streaking so
18:56
I'm not sure how normal that is this is
18:58
on fairly bright scene looking out the
19:02
window if I cut the exposure time down
19:04
on that it's now 1 second
19:07
exposure again most of the image
19:09
disappears again this is looks like it's
19:11
possibly over still overloading here go
19:14
that go down to say say quarter a
19:16
second so again I think there might be
19:19
some Auto gain control going on here um
19:21
this is with the PFG option let's try
19:23
turning that off and see what
19:25
happens so I'm not sure this is actually
19:27
more streaking or which just it's
19:29
cranked up the gain all the dis display
19:31
gray scale to show what um you know the
19:33
range of things that it's captured
19:36
there's one of one of 12 things in the
19:38
software there's um you can see of you
19:40
can't seem to read out the temperature
19:42
of the pelta cooler but you can set the
19:44
temperature and if you said it's a
19:46
different temperature you see the power
19:48
consumption jump up running the cooler
19:50
to get the temperature you requested but
19:52
I can't see anything anywhere that tells
19:54
you whether the cool is at the at the
19:56
temperature other than the power
19:57
consumption going down and there's no
19:59
temperature read out
20:03
here and just some yeah this is just
20:05
sort of very basic software I'm sure
20:07
there's like an API for more
20:09
sophisticated
20:10
applications but so if you know anything
20:12
more about these cameras please um stick
20:14
in the
20:15
comments um incidentally when I was
20:18
editing I didn't notice there was a bent
20:19
pin on the um CCD but I did fix that
20:22
before doing these tests and also
20:24
reactivated the um silica gel desicant
20:26
cuz I noticed it was uh I was getting
20:28
bit of condensation on the window but um
20:31
yeah so a couple of uh interesting but
20:34
maybe not particularly uh useful pieces
20:37
of Kit except for someone that's got a
20:38
very specific use so um I'll stick a
20:42
I'll stick these on eBay put a link in
20:44
the description and say hopefully
20:45
someone could actually make some uh good
20:47
use of these things
Example Output:
**Abstract:**
This video presents Part 2 of a teardown focusing on the optical components of a Fluidigm Polaris biotechnology instrument, specifically the multi-wavelength illuminator and the high-resolution CCD camera.
The Lumen Dynamics illuminator unit is examined in detail, revealing its construction using multiple high-power LEDs (430nm, 475nm, 520nm, 575nm, 630nm) combined via dichroic mirrors and filters. A square fiber optic rod is used to homogenize the light. A notable finding is the use of a phosphor-converted white LED filtered to achieve the 575nm output. The unit features simple TTL activation for each color, conduction cooling, and internal homogenization optics. Analysis of its EEPROM suggests extremely low operational runtime.
The camera module teardown showcases a 50 Megapixel ON Semiconductor KAF-50100 CCD sensor with micro-lenses, cooled by a multi-stage Peltier stack. The control electronics include an FPGA and a USB interface. Significant post-manufacturing modifications ("bodges") are observed on the camera's circuit boards. Basic functional testing using vendor software and a pinhole lens confirms image capture but reveals prominent vertical streaking artifacts, the cause of which remains uncertain (potential overload, readout artifact, or fault).
**Exploring the Fluidigm Polaris: A Detailed Look at its High-End Optics and Camera System**
* **0:00 High-End Optics:** The system utilizes heavy, high-quality lenses and mirrors for precise imaging, weighing around 4 kilos each.
* **0:49 Narrow Band Filters:** A filter wheel with five narrow band filters (488, 525, 570, 630, and 700 nm) ensures accurate fluorescence detection and rejection of excitation light.
* **2:01 Customizable Illumination:** The Lumen Dynamics light source offers five individually controllable LED wavelengths (430, 475, 520, 575, 630 nm) with varying power outputs. The 575nm yellow LED is uniquely achieved using a white LED with filtering.
* **3:45 TTL Control:** The light source is controlled via a simple TTL interface, enabling easy on/off switching for each LED color.
* **12:55 Sophisticated Camera:** The system includes a 50-megapixel Kodak KAI-50100 CCD camera with a Peltier cooling system for reduced noise.
* **14:54 High-Speed Data Transfer:** The camera features dual analog-to-digital converters to manage the high data throughput of the 50-megapixel sensor, which is effectively two 25-megapixel sensors operating in parallel.
* **18:11 Possible Issues:** The video creator noted some potential issues with the camera, including image smearing.
* **18:11 Limited Dynamic Range:** The camera's sensor has a limited dynamic range, making it potentially challenging to capture scenes with a wide range of brightness levels.
* **11:45 Low Runtime:** Internal data suggests the system has seen minimal usage, with only 20 minutes of recorded runtime for the green LED.
* **20:38 Availability on eBay:** Both the illuminator and camera are expected to be listed for sale on eBay.
Here is the real transcript. What would be a good group of people to review this topic? Please summarize provide a summary like they would:
00:00:06 Hello, it's Scott Manley here. Over the
00:00:06 years, I've made a lot of videos about
00:00:09 rocket engines, the devices which
00:00:11 harness the intense energy of chemical
00:00:13 combustion to propel rockets into space,
00:00:16 but I have never talked about the flip
00:00:18 side of this, the risks of fire during
00:00:21 human space flight. The US's first real
00:00:24 disaster in space flight is of course
00:00:25 the Apollo 1 fire and that was a tragic
00:00:28 illustration of the danger of fire in a
00:00:31 confined space with a pure oxygen
00:00:33 environment. It caused a pause and a
00:00:35 re-evaluation of the Apollo program and
00:00:38 in turn the rest of the program likely
00:00:40 benefited from the changes that came out
00:00:42 of this terrible event. But the Apollo
00:00:44 on fire isn't really what this video is
00:00:47 about. For a start, people on the
00:00:48 internet regularly hear me talking about
00:00:51 pure oxygen atmospheres in space suits,
00:00:53 and they draw a direct line to Apollo 1.
00:00:55 But this misses the effect of the
00:00:58 atmospheric pressure. Apollo 1 had an
00:01:00 atmospheric pressure of 33% more than
00:01:03 sea level, whereas pure oxygen
00:01:06 atmospheres and space suits are
00:01:07 typically 1/3 of the pressure at sea
00:01:10 level. So they are a lot safer. So
00:01:13 anyway, yeah, this is more concerning
00:01:15 fires in zero gravity in a confined
00:01:18 space. The way fire behaves in the
00:01:20 absence of gravity is hugely different
00:01:22 from what we might deal with on Earth.
00:01:25 The hazards are different and the best
00:01:27 way to fight it has to account for the
00:01:29 fact that you can't just throw the
00:01:30 burning material overboard. In
00:01:32 particular, a few people asked about the
00:01:34 new NASA policy allowing smartphones on
00:01:37 the space station. Many people know that
00:01:39 lithium ion batteries can suffer a
00:01:42 thermal runaway process when they're
00:01:44 damaged and wondered how astronauts
00:01:46 would deal with such a situation to stop
00:01:48 it spreading. First things first, why
00:01:52 does fire act so strangely without
00:01:54 gravity? Well, down here on Earth,
00:01:56 buoyancy rules the day. Hot gases
00:01:58 expand. They become less dense than the
00:02:01 surrounding air, and that means they
00:02:03 rise, pulling in fresh air from below
00:02:05 through convection. That's why, you
00:02:07 know, I have a campfire with a classic
00:02:08 pointed shape, which they burn hot and
00:02:11 fast. Now, in microgravity, though,
00:02:13 there's no buoyancy. There's no air
00:02:15 rising. Everything is weightless. The
00:02:17 flames form a sort of spherical uh area
00:02:21 around the hot spot or like a gentle
00:02:23 dome shape on the surface. Oxygen only
00:02:26 reaches the fuel by diffusion, which is
00:02:28 a slow random bumping process of
00:02:30 molecules. The result is that flames
00:02:33 that will burn slower and cooler while
00:02:35 the air flow moves in slow and
00:02:38 interesting ways. One upshot of this
00:02:40 slow combustion is that the flame can
00:02:42 sustain at much lower levels of oxygen
00:02:44 in zero gravity than would work on
00:02:47 Earth. So NASA has been studying this uh
00:02:50 flames in zerog for years with
00:02:52 experiments like Flex 2, the flame
00:02:54 extinguishment extinguishment experiment
00:02:57 where they ignite tiny fuel droplets in
00:03:00 the combustion integrated rack on the
00:03:02 ISS. These spherical flames sometimes
00:03:04 pulse like jellyfish or even reveal cool
00:03:07 flames, dim almost invisible afterglows
00:03:10 that are actually still burning long
00:03:12 after you think the fire's out. Other
00:03:14 projects like Acme and Sophie, the solid
00:03:17 fuel ignition and extinction test at
00:03:20 real materials, fabrics, plastics, and
00:03:22 wiring, and they show how flames can
00:03:24 creep along surfaces in unexpected ways,
00:03:27 sometimes even spreading against the air
00:03:29 flow caused by the forced ventilation
00:03:32 from the station's fans. More recently,
00:03:35 NASA has been doing larger scale
00:03:37 experiments, namely space flight
00:03:39 aircraft fire safety experiment or
00:03:41 Sapphire. These were bigger and by
00:03:44 extension more dangerous than the
00:03:46 experiments which had been run on the
00:03:47 ISS and so they used an interesting
00:03:49 mission plan. They would run on the
00:03:52 Signis cargo spacecraft after it had
00:03:54 left the station on its way to disposal
00:03:56 at the end of its mission. If the fire
00:03:58 somehow got out of control, it would
00:04:00 only affect a spacecraft that was about
00:04:02 to be destroyed anyway. These
00:04:04 experiments could look at larger scale
00:04:06 propagation of flames along combustible
00:04:08 materials which might be found on the
00:04:11 ISS.
00:04:13 Anyway, without gravity to help vent
00:04:15 combustion products, CO2 and water vapor
00:04:19 build up around the flame. Uh the
00:04:21 potentially smothering the flame, unless
00:04:23 of course the spacecraft has air
00:04:25 circulation that just keeps feeding it
00:04:26 enough oxygen to keep going. The flame
00:04:29 can be slower than a fire on the Earth,
00:04:31 sure, but it can be much sneakier. A
00:04:34 smoldering wire behind a panel could go
00:04:36 unnoticed for hours before it finally
00:04:39 flares up. Lower temperature combustion
00:04:41 also means that the combustion is less
00:04:43 complete, less clean. So, there's all
00:04:46 sorts of molecules that don't break down
00:04:48 as fully as they would on Earth. And as
00:04:50 a result, fires burn with more suit and
00:04:53 nasty molecules come off. And this means
00:04:55 that in general, if there is a fire in a
00:04:57 spacecraft, the biggest danger to the
00:04:59 crew isn't going to be the heat and the
00:05:01 flames. It's going to be the smoke and
00:05:04 the chemicals escaping and contaminating
00:05:06 the atmosphere faster than the
00:05:08 environmental control system can clean
00:05:10 it up. In zero gravity, smoke doesn't
00:05:13 rise or layer. It spreads out evenly
00:05:16 throughout the module, following the
00:05:18 ventilation paths, and it hangs around a
00:05:20 lot longer. There's a lot of combustion
00:05:22 products that can be really dangerous to
00:05:24 humans. For example, carbon monoxide,
00:05:28 right? This pretty much comes from
00:05:30 incomplete combustion of carbon
00:05:31 products. It sneaks around silently. It
00:05:34 binds to your blood and basically messes
00:05:37 up your hemoglobin, starving your brain
00:05:39 for oxygen. This leads to headaches,
00:05:41 confusion, or worse. You can get
00:05:43 hydrogen cyanide from burning plastics.
00:05:45 And again, that is a neurotoxin. It
00:05:47 shuts down cellular respiration and it
00:05:49 causes rapid unconsciousness. Hydrogen
00:05:52 chloride and hydrogen fluoride can be
00:05:54 evolved from polymers like teflon or
00:05:57 PVC. These form acid on contact with
00:06:00 moisture and they get absorbed through
00:06:02 the skin while poisoning your system.
00:06:04 Particulates like soot or metal residues
00:06:07 like nickel and cobalt from batteries.
00:06:09 They can get deep into your lungs and
00:06:11 damage the surface potentially setting
00:06:13 the stage for things like chronic
00:06:15 obstructive pulmonary disease. Over time
00:06:18 in a closed loopa spacecraft these
00:06:20 toxins don't dissipate and they build up
00:06:22 and life support scrubbers can get
00:06:24 overwhelmed and take too long to clean
00:06:26 the air. Now again all of this is well
00:06:28 studied through experiments but the one
00:06:30 really good example of a fire in space
00:06:33 flight doesn't deal with any of these
00:06:35 strange zerog behaviors because it was a
00:06:38 fire that generated its own oxygen. This
00:06:41 video is sponsored by Incogn. So let me
00:06:43 introduce you to my patch collection.
00:06:45 These are patches from places I've been,
00:06:47 people I've met, and I like to put them
00:06:48 on display. And if you look, you can put
00:06:50 together a picture of the things I've
00:06:52 done. And I know there are some of you
00:06:54 already out there zooming in. And while
00:06:56 this is all in good fun, it's actually a
00:06:58 great metaphor for a real problem that
00:07:00 lots of us deal with. There are
00:07:02 companies who make it their business to
00:07:03 collect clues like this from various
00:07:05 sources to build up pictures of people's
00:07:07 lives. People like you. You may have
00:07:09 seen websites that offer to help you
00:07:12 find information on people. Things like
00:07:13 addresses and phone numbers can be
00:07:15 bought for a price. Your personal
00:07:17 information is for sale by data brokers
00:07:19 to anyone that wants to buy it, whether
00:07:21 they be marketers, fraudsters, or
00:07:22 timetraveling cyborgs from the future.
00:07:25 And you can imagine all that misuse of
00:07:27 information has a high potential for bad
00:07:29 things. In one case, a fraudster used
00:07:31 data they bought to pose as individuals
00:07:33 and get loans in their name, taking the
00:07:35 money and leaving the victim to deal
00:07:37 with the fallout. And so today's
00:07:38 sponsor, Incogners a way to protect
00:07:40 yourself from this kind of investigation
00:07:42 where they will get the data dealing
00:07:44 websites to remove your data. There are
00:07:46 laws that protect you from this kind of
00:07:47 thing, but it takes a lot of time and
00:07:49 incognies and speeds up the removal
00:07:51 process with a fully automated system
00:07:53 dedicated to the task of restoring your
00:07:56 privacy. It's easy to set up. Create
00:07:58 your account and give them the
00:07:59 information they need to identify you.
00:08:01 And then you'll see a huge number of
00:08:02 matches from sources across the web.
00:08:04 Then with your permission, they will
00:08:06 send out takedown requests on your
00:08:07 behalf, scrubbing the internet of your
00:08:09 secrets. Sometimes you'll find
00:08:11 information outside the hundreds of
00:08:13 covered sites. And that's fine because
00:08:14 Incogn offers a custom removal feature
00:08:16 that lets you use their automated tools
00:08:18 to address the removal of your secrets
00:08:20 from websites almost anywhere. So take
00:08:23 back your personal data within Cognney.
00:08:25 Use code Manley at the link in the
00:08:27 description to get 60% off an annual
00:08:29 plan. And now back to the video. So now
00:08:33 February 23, 1997,
00:08:36 we are on the Mir space station and Mir
00:08:38 was already an aging beast. It was a
00:08:40 patchwork of modules orbiting for over a
00:08:42 decade. Uh at this point there were two
00:08:45 suses dopped with six crew members on
00:08:48 board commanded by Valerie Kurzen. There
00:08:50 was also a guest astronaut from Germany,
00:08:52 Reinhald Eidwald and NASA's Jerry
00:08:55 Lininger was there and it was a relaxed
00:08:57 evening. They had uh you know sausages,
00:08:59 cheese, caviar in the base block and
00:09:02 then uh one of the cosminauts gets the
00:09:04 job of swapping in a solid fuel oxygen
00:09:07 generator candle in the Cavant one
00:09:09 module. With a crew of six, the station
00:09:11 needed extra oxygen to keep the air
00:09:13 breathable. So they would burn one of
00:09:15 these three times a day. These are
00:09:17 lithium perchlorate canisters and they
00:09:19 release oxygen through a simple
00:09:20 controlled burning is the chemistry is
00:09:22 that lithium perchlorate breaks down to
00:09:25 give you breathable oxygen plus lithium
00:09:27 chloride. And this is an exothermic
00:09:29 process that's usually contained inside
00:09:31 the canister casing. They get mounted
00:09:33 and then when activated the chemistry
00:09:35 kicks off and the canister emits a
00:09:38 steady stream of oxygen for the next 20
00:09:40 minutes until it's spent. This is the
00:09:42 same oxygen generation process that's
00:09:44 used in airliners for those passenger
00:09:46 cabin oxygen masks. This is a well
00:09:48 understood and widely deployed
00:09:50 technology. Prior to this, the canisters
00:09:52 had been used without incident over 2500
00:09:55 times. It was a routine operation, but
00:09:57 as you can guess, this one time was not
00:10:00 routine. Right? When the canister was
00:10:02 activated, the exothermic reaction
00:10:04 became more rapid than expected. And the
00:10:06 best theory is that during production, a
00:10:08 piece of latex glove used in the
00:10:10 manufacturing process ended up inside
00:10:13 the canister. And this burned with the
00:10:15 excess oxygen at a high enough
00:10:17 temperature that it caused the aluminium
00:10:19 casing to melt and start burning itself.
00:10:22 So an orange fra flame began escaping
00:10:25 the canister and it quickly grew to 3 ft
00:10:28 long jet blowing molten sparks of
00:10:30 aluminium out into the cabin, melting
00:10:33 cables, scorching the walls. There was a
00:10:35 worry that the hull of the station might
00:10:36 have been compromised, leading to
00:10:38 pressure being lost. But thankfully, the
00:10:41 flame was being emitted away from the
00:10:42 walls into the middle of the module. But
00:10:45 this zerog fire wasn't a quiet low
00:10:48 temperature jellyfish hunting for
00:10:50 oxygen. The self oxidizing reaction made
00:10:53 it burn hot and directional like a
00:10:55 blowtorrch. Smoke was thick, acrid,
00:10:58 laced with hydrogen chloride, flooding
00:11:00 out all over the place, and visibility
00:11:03 dropped to the point where the crew
00:11:04 could barely see their own hands. And
00:11:07 because it was a jet of flame across the
00:11:09 middle of the module, it blocked access
00:11:11 to one of the Soyu spacecraft, cutting
00:11:13 off half the crew from their escape
00:11:15 route should the worst happen. Alarms
00:11:18 were triggered automatically as the
00:11:19 smoke detectors picked up the particles.
00:11:21 The crew were supposed to dawn oxygen
00:11:24 masks as a first step. And NASA
00:11:26 astronaut Jerry Lininger remembers
00:11:28 grabbing the nearest mask, putting it on
00:11:30 and taking a breath and realizing he
00:11:33 wasn't getting oxygen. And that left him
00:11:34 holding his breath for a long time until
00:11:37 he could find a working mask. By the
00:11:39 time Jerry had a working mask, the
00:11:41 station commander, Valeri Kerzone, was
00:11:43 actively working to suppress a fire
00:11:45 using fire extinguishers on the station,
00:11:48 which were water foam extinguishers. It
00:11:50 had taken longer than expected to deploy
00:11:52 the fire extinguishers cuz the brackets
00:11:54 holding them to the wall were locked
00:11:56 closed with bolts so that the
00:11:58 extinguishers wouldn't fall out during
00:12:00 the launch. Somehow nobody had got
00:12:02 around to removing the bolts. The fire
00:12:05 extinguishers had two modes. They could
00:12:06 generate foam or they could just spray
00:12:08 water. It appeared that the foam mode
00:12:10 wasn't useful in this particular case.
00:12:12 the foam wasn't in stay staying in place
00:12:14 because the canister was generating
00:12:17 extra gas rather than consuming
00:12:19 atmospheric oxygen. So yeah, they used
00:12:22 the old-fashioned water mode on the fire
00:12:24 extinguisher. And even with the
00:12:26 extinguishers, it was impossible to
00:12:28 actually stop this fire because it was
00:12:29 generating its own oxygen. But the water
00:12:33 did have the effect of cooling the flame
00:12:36 down to limit its ability to spread and
00:12:38 cause damage to critical systems. So
00:12:41 when you're using a fire extinguisher in
00:12:43 zerog, there is inevitably a thrust from
00:12:46 the fluid being sprayed out. And so the
00:12:48 other crew members had to work with
00:12:50 Valeri to brace him and pass him more
00:12:52 fire extinguishers as he expended them.
00:12:55 And I believe by the time they had this
00:12:57 under control, they had used three fire
00:12:59 extinguishers with one as another one
00:13:01 not actually working. In the process,
00:13:04 Corzan re received significant burns on
00:13:06 his hands and chest from blobs of molten
00:13:09 metal floating around in the cabin.
00:13:12 There was concerns that the burns to his
00:13:13 hand might actually make it impossible
00:13:15 for him to dawn his suit gloves and
00:13:17 operate the soy use for return to Earth.
00:13:20 So while the fire was ultimately
00:13:22 extinguished, the smoke would linger for
00:13:24 hours. And the environmental control
00:13:26 system did work to clear the air slowly,
00:13:28 but a lot of the black smoke actually
00:13:30 ended up being mopped up as the excess
00:13:33 water from the extinguishers condensed
00:13:35 on the station's walls. The crew would
00:13:38 spend hours mopping up black water from
00:13:40 the walls of the station using discarded
00:13:42 clothes.
00:13:44 So Russia's response of course was to
00:13:46 minimize the report, initially claiming
00:13:48 that the fire was extinguished in less
00:13:50 than 90 seconds when in fact the fire
00:13:53 continued to burn for at least 15
00:13:55 minutes. It also later transpired that
00:13:57 another fire with an oxygen generator
00:13:59 had occurred on mere 3 years earlier in
00:14:02 1994. And this hadn't been reported to
00:14:05 NASA at the time, although this prior
00:14:07 incident wasn't nearly so
00:14:08 life-threatening. It wasn't even the
00:14:11 first fire on a Soviet built station.
00:14:13 Salute 1 had a small electrical fire
00:14:16 which was never visible, but it
00:14:18 contaminated the air. The crew's only
00:14:20 real way of dealing with this was to cut
00:14:22 down cut off power to the systems until
00:14:25 they thought the problem had been
00:14:27 solved, but they weren't sure. On Salute
00:14:30 6 in 1977, an electrical fire in a
00:14:33 control system was a significant
00:14:35 emergency. The mission commander was
00:14:36 Vladimir Kavalionok and he later
00:14:39 provided a firsthand account of the
00:14:41 situation. We have a navigation complex
00:14:45 on board and there was a testing
00:14:47 program. Without her approval, the
00:14:49 control center was turning it on and
00:14:51 off. Kavalionok and his flight engineer
00:14:54 Alexander Ivanchenkov were exercising
00:14:57 after listening to a concert. Suddenly,
00:14:59 Ivanchkov noticed a burst of smoke and
00:15:02 pl flames from the control panel. We
00:15:04 started to fight the fire, switching off
00:15:06 a number of systems. They switched off
00:15:08 all of the fans in order to stop the air
00:15:11 supply to the fire. Kavalionok then
00:15:14 grabbed the foam extinguisher and
00:15:17 sprayed the burning unit. We took all
00:15:19 the necessary precautions. We were ready
00:15:21 to abandon the station, he added. There
00:15:24 were plenty of toxic gases in the air.
00:15:27 We used gas masks to continue our work.
00:15:30 Now, previous NASA missions had various
00:15:33 firefighting options on board. The water
00:15:35 dispenser on the Apollo spacecraft
00:15:37 intended for food and drinks was
00:15:39 considered an option, but it was never
00:15:41 really needed in this capacity, which is
00:15:43 good because they actually tested it in
00:15:45 experiments on Skyab, and they showed
00:15:47 that it was hard to reliably aim the
00:15:49 relatively slow flow of water, and the
00:15:51 stream of water wasn't very good at
00:15:53 tackling fires even when it was aimed
00:15:55 correctly. The Apollo program did
00:15:57 develop a foam fire extinguisher using
00:16:00 freon and nitrogen and the deployment
00:16:02 and foaming was demonstrated on Skylab
00:16:05 but it was never actually needed uh or
00:16:07 ever tested against a real fire in zero
00:16:10 gravity. Now the space shuttle, it
00:16:13 looked to its aviation routes and it
00:16:15 included halon fire extinguishers
00:16:17 derived from those used on jet aircraft.
00:16:20 And for example, the instrument panels,
00:16:22 they incorporated special ports where
00:16:24 the fire extinguishers could inject
00:16:26 their fire suppressant into the panels
00:16:28 should there be an electrical fire
00:16:29 inside of those. The space lab and the
00:16:32 space hab payloads also included a
00:16:35 general halon firefighting system which
00:16:37 could flood the whole unit in an
00:16:38 emergency.
00:16:40 However, the downside to the halon
00:16:42 systems is that the reaction products
00:16:44 which uh resulted were not easy to
00:16:46 remove by the shuttle's environmental
00:16:48 control system. And so the mission plan
00:16:50 would require that an an emergency
00:16:52 landing of the shuttle at the first
00:16:54 opportunity within a few hours if the
00:16:57 fire extinguishers were ever used. And
00:16:59 of course with a space station, you
00:17:01 can't force an emergency landing. So you
00:17:04 need to change the type of extinguishers
00:17:06 that are used away from these halon
00:17:08 gases. So now back to the present day.
00:17:11 Uh detection systems on modern stations
00:17:13 like the ISS are much smarter than what
00:17:15 we had. Smoke is the focus because cool
00:17:18 flames mean less heatness signature and
00:17:20 the particles tend to you know stick
00:17:22 around. So they have laserbased
00:17:24 detectors that trigger on soup particles
00:17:27 scattering light. And these are located
00:17:28 in vents and open areas sniffing for
00:17:31 micronsized particles with some
00:17:33 detectors actively pulling air in so
00:17:35 they can get a rapid warning. There's
00:17:37 about 30 of these detectors across the
00:17:39 US segments and all the alarms feed into
00:17:42 the station's control system. When one
00:17:44 triggers a crew, a crew member can
00:17:46 pinpoint the location using the station
00:17:48 management laptops. So alarms will
00:17:51 trigger automatic vent shutdowns and
00:17:53 power cuts in affected modules and
00:17:55 operators in mission control can
00:17:57 manually intervene even if the crew on
00:17:59 orbit is sleeping and taking a few
00:18:01 moments to get into action. There are
00:18:03 also gas analyzers are tracking specific
00:18:05 contaminants which are known toxins.
00:18:07 Again, carbon monoxide, hydrogen
00:18:10 cyanide, hydrogen chloride. The crew
00:18:13 response to fight the fire then follows
00:18:15 a drilled sequence. When the alarm hits,
00:18:18 everybody has to get on portable
00:18:19 breathing apparatus, which are full face
00:18:22 masks, which have you 15 to 30 minutes
00:18:25 worth of oxygen and they carry small
00:18:27 oxygen bottles for mobility.
00:18:30 Then the crew may take further decisions
00:18:32 to shut down ventilation and power in
00:18:35 the affected areas to limit air flow and
00:18:37 slow the fire. Mission control may
00:18:39 already have taken action, but the crew
00:18:41 on orbit have a firsterson understanding
00:18:44 of what the situation is. Then the crew
00:18:47 can actually work on suppressing the
00:18:48 fire with portable fire extinguishers.
00:18:50 So in the US segment, they don't use
00:18:52 foam extinguishers. They don't have
00:18:54 those halon extinguishers anymore.
00:18:56 Instead, they have CO2 extinguishers.
00:18:59 And there were 13 of these initially
00:19:01 launched on this or deployed throughout
00:19:02 the station. CO2 was chosen because of
00:19:06 experience on the earth with electrical
00:19:08 fires and because liquid water-based
00:19:10 extinguishers uh the water has a
00:19:12 tendency to collect into balls rather
00:19:14 than cover the fire in zerog
00:19:17 and carbon dioxide works with the ST
00:19:20 space station's life support system
00:19:21 which is designed to remove carbon
00:19:23 dioxide from the atmosphere. But on the
00:19:26 other hand, carbon dioxide in the
00:19:27 atmosphere is not great for the
00:19:28 astronauts. So it's not necessarily the
00:19:31 best option to be fighting a fire with
00:19:33 this. Now later a second type of fire
00:19:35 extinguisher was developed for space
00:19:37 flight. And these have replaced many of
00:19:39 the CO2 extinguishers on the station.
00:19:41 These are designed to emit a fine water
00:19:44 mist. Fine enough that the water doesn't
00:19:46 collect into big globules as it spreads
00:19:48 out. The water mist systems creates a
00:19:50 fog of micronsized droplets that quickly
00:19:53 remove the heat and replace oxygen as
00:19:56 the water evaporates, suppressing the
00:19:58 fire and preventing it from spreading to
00:20:00 other surfaces. So water is a lot better
00:20:02 than CO2 because it takes a lot more to
00:20:05 interfere with the human respiratory
00:20:07 system than CO2.
00:20:10 Secondly, it's more effective at cooling
00:20:12 the fire. And this would make it
00:20:14 effective against an oxygen generator
00:20:16 fire, but also against, say, lithium-ion
00:20:19 battery fires, which of course brings me
00:20:21 back to what might happen if a device
00:20:24 with a modern highdensity lithium ion
00:20:27 battery experienced a thermal runaway on
00:20:30 the space station. This is a concern on
00:20:32 passenger aircraft. Now, many of you
00:20:34 will remember hearing airlines banning
00:20:36 certain models of Samsung phones because
00:20:39 of an unusually high rate of battery
00:20:41 failures. Now, thankfully, Samsung has
00:20:44 since fixed this problem, but people
00:20:46 remember the problems of fires in
00:20:48 aircraft cabins. So, aircraft cabin
00:20:50 equipment now includes firebags, which
00:20:52 cabin crew can be used to isolate
00:20:55 burning devices or ideally devices that
00:20:57 are just getting very hot before they
00:20:59 actually catch fire. And I imagine that
00:21:01 it would make sense if this kind of gear
00:21:03 was deployed on the ISS, but I haven't
00:21:05 found anything specific. But the water
00:21:08 mist fire extinguisher, well, it won't
00:21:10 be able to put out the fire because this
00:21:12 is a chemical reaction which is internal
00:21:13 to the battery. But the water will cool
00:21:16 the reaction and absorb more of the
00:21:18 evolved gases and smoke, helping to
00:21:20 reduce the contamination of the
00:21:22 spacecraft's atmosphere. And again,
00:21:24 modern consumer electronics just love to
00:21:27 include fluorinated polymers for their
00:21:29 stability under normal conditions. But
00:21:31 yet, when they break down, that creates
00:21:33 hydrogen fluoride, which is terrible for
00:21:35 humans. So, on the space station, if a
00:21:37 fire is not safe to tackle, the crew
00:21:39 does have the option of closing the
00:21:40 hatches to the module. But this is
00:21:42 primarily to contain the smoke and
00:21:44 reduce contamination through the rest of
00:21:46 the station. And of course, closing the
00:21:48 hatches will reduce the air flow and
00:21:50 ultimately reduce the available oxygen
00:21:52 until the combustion stars of oxygen
00:21:54 itself limits. But there's a classic
00:21:56 trope in science fiction where you can
00:21:59 fight fires by depressurizing a
00:22:01 spacecraft or just an affected portion
00:22:03 of the spacecraft. Now, clearly this
00:22:06 works according to the laws of physics,
00:22:07 but as far as I know, there's no point
00:22:09 in the checklist where astronauts would
00:22:11 resort to this. Many of the station
00:22:13 modules do actually have limited ability
00:22:15 to vent atmosphere for things like
00:22:17 experiments and racks, but this isn't
00:22:19 something that you're able to do from
00:22:20 outside the module as far as I can tell.
00:22:22 Some modules may have been designed with
00:22:24 this capability, but it's not universal.
00:22:27 And the space station procedures for
00:22:29 this kind of eventuality
00:22:31 uh are not public. So I wouldn't know if
00:22:33 this is actually a procedure that can be
00:22:35 done. The thing is 99% of the work of
00:22:38 fighting fires in spaceflight is on the
00:22:41 prevention side. eliminating ignition
00:22:43 sources and choosing materials which are
00:22:45 fireresistant. There's a huge amount of
00:22:47 materials testing and validation that's
00:22:49 performed in labs on the ground to make
00:22:51 sure that the things that are sent to
00:22:53 space aren't going to have a hidden
00:22:55 danger. The testing includes atmospheres
00:22:57 with higher concentrations of oxygen
00:22:59 which can occur under some conditions on
00:23:02 the station ensuring that they are
00:23:03 testing for the worst case scenarios. An
00:23:06 example of a material which is common
00:23:08 and needs special treatment is Velcro,
00:23:11 right? or in NASA terminology, hook and
00:23:13 loop fasteners. And it's pretty common
00:23:15 in space flight because it's great at
00:23:17 holding things down that would otherwise
00:23:19 float around. This material was cited as
00:23:21 one of the problems in the Apollo 1
00:23:23 fire. And while it's not been eliminated
00:23:26 in space flight, they do have a fire
00:23:28 retardant version of Velcro, right,
00:23:30 which is used in spacecraft and
00:23:32 aviation, obviously. Furthermore,
00:23:34 there's NASA specifications that limit
00:23:36 patches of Velcro to no more than four
00:23:39 square in. Uh, another article I found
00:23:42 discussed the replacement of
00:23:43 old-fashioned polyine uh, trash bags
00:23:47 with a new fireresistant material known
00:23:49 as Armor Flex 301. The active station
00:23:52 had been accumulating lots of trash in
00:23:54 bags and the bags being flammable was
00:23:57 becoming to be considered a significant
00:23:59 hazard. On the other hand, of course,
00:24:01 one unintended consequence of this focus
00:24:03 on nonflammable materials is yes, a lot
00:24:06 of materials have had a teflon and stuff
00:24:10 replacing regular plastic, which again
00:24:12 causes problems because of those hot
00:24:14 flurinated molecules breaking out and
00:24:16 making hydrogen fluoride. Regardless,
00:24:19 this focus on fire prevention has
00:24:21 obviously paid off given that in the 25-
00:24:23 year history of the space station, we
00:24:26 have not seen any unplanned fires that
00:24:29 are outside of the equipment racks.
00:24:31 Nothing has escaped the racks and caused
00:24:33 any trouble for the crew. But now we're
00:24:35 in a situation we are looking towards
00:24:38 the future with a potential return to
00:24:40 the moon and maybe Mars. Right? The
00:24:42 safety engineers planning for these
00:24:44 environments will once again have to
00:24:45 account for habitable spaces which
00:24:47 experience gravity and these spaces will
00:24:50 also have to experience zero gravity for
00:24:52 some of the time and they will have to
00:24:54 be fires safe for both of these. This
00:24:55 changes the way that fire burns in a
00:24:58 gravity and and that means you have to
00:25:00 change the way your fire suppression
00:25:02 systems operate. the smoke detectors
00:25:04 will have to pay attention to where the
00:25:05 top of the cabin is so that the rising
00:25:08 smoke moves towards detectors and not
00:25:10 away from them. And if we want to look
00:25:12 to an even more distant future, imagine
00:25:15 a human mission to Titan where the
00:25:17 spacecraft of course has an oxygen
00:25:19 atmosphere inside, but as soon as you
00:25:20 open the door, you are having
00:25:22 potentially combustible hydrocarbons
00:25:24 coming in. That will require another
00:25:27 iteration on spaceflight safety with
00:25:30 regards fire. I'm Scott Manley. Fly