<p><strong>TL;DR: Not all life requires atmospheric oxygen or carbon dioxide. There are many organisms here on Earth that use <a href="https://en.wikipedia.org/wiki/Chemosynthesis" rel="nofollow noreferrer">chemosynthesis</a> to process chemicals like methane or hydrogen sulphide for energy.</strong></p>

<hr>

<p>The search for life on Mars has concentrated on finding evidence of <a href="https://en.wikipedia.org/wiki/Autotroph" rel="nofollow noreferrer">autotrophic</a> microorganisms – organisms that convert simple chemicals in the environment into complex organic compounds. Most autotrophs use water as the reducing agent, but some can use other chemicals like hydrogen sulphide. </p>

<p>The energy source for these autotrophs can either be sunlight, in which case we call them <a href="https://en.wikipedia.org/wiki/Phototroph" rel="nofollow noreferrer"><em>phototrophs</em></a> (which includes algae and green plants here on Earth), or obtained through the oxidation of electron donors in their environment, in which case they're called <a href="https://en.wikipedia.org/wiki/Chemotroph" rel="nofollow noreferrer"><em>chemotrophs</em></a>. </p>

<p>There's a wide variety of chemotrophs here on Earth, typically living in completely dark and often hostile environments such as next to deep-sea volcanic vents. For example, iron-oxidizing bacteria even colonise new lava beds in the deep ocean, and in effect use the oxidation of available ferrous iron as their respiratory process.</p>

<p>There's no reason to think that autotrophs couldn't find niche environments on Mars in which to exist, but the biggest hurdles are the significantly lower temperature and pressure, and the significantly greater radiation. The latter can be overcome by colonising <em>sub-surface</em> environments, which eliminates the phototrophs from contention. While UV radiation penetrates soils only in the millimetre range, <a href="http://discovery.ucl.ac.uk/134609/1/2006GL027494.pdf" rel="nofollow noreferrer">one study</a> found that viable dormant cells would have to be at least 7.5m below the planet's surface to survive the cumulative damage from cosmic radiation.</p>

CC BY-SA 4.0
2018-11-22T00:31:38.157Z
2018-11-22T00:31:38.157Z
Chappo Hasn't Forgotten
<p>What's more, in addition to finding potential evidence for life now, there is also the equally important possibility of past life that has gone extinct but left biosignatures like fossils or other geological byproducts.  It is important to realize that there is considerable evidence that the Martian climate used to be very different, and there may have been a much denser atmosphere, providing the carbon dioxide that plant life would need to live on the surface and use photosynthesis.  The fact that there is not a lot of oxygen in the atmosphere now suggests that there was not a multibillion year history of plant life like the Earth has (a lot of it without much oxygen), but there could have been a short period where life did thrive, and it might be hard to tell now that this ever happened-- without looking closely.  But yes, it does seem likely that there are places in the galaxy more conducive to life than Mars, Mars is just the closest-- and you always start looking for your lost keys under the streetlights, going on only after you've eliminated that possibility.</p>

CC BY-SA 4.0
2018-11-22T09:04:52.153Z
+1 for the additional detail! A denser atmosphere historically would address the problems with temperature and especially pressure (current pressure is too low for almost all cellular life), but I'm guessing would have a negligible impact on cosmic radiation, so I'm not sure that phototrophs would have been viable?
Chappo Hasn't Forgotten
CC BY-SA 4.0
2018-11-22T09:26:35.807Z
You mean the fact that Mars has little magnetic field to protect against energetic particles?  It might cause a lot of genetic damage, but would it sterilize the planet?  It is thought interaction with perchlorates might produce toxic surface compounds, so you may be right.
Ken G
CC BY-SA 4.0
2018-11-22T10:32:23.497Z
It's the cumulative genetic damage from energetic particles - see the link in last para of my post. The perchlorate problem is exacerbated by *UV* rather than energetic particles, and despite a quick search, I can't find if UV is absorbed by CO2. I'm assuming CO2 is only opaque to the longer IR wavelengths.
Chappo Hasn't Forgotten
CC BY-SA 4.0
2018-11-22T08:50:04.267Z
2018-11-22T08:50:04.267Z
Ken G
<p>If all living things like animals require oxygen to live, how can people think that there could be life on other planets such as mars for example ? Living things require oxygen and carbon dioxide, and these planets do not have plants and such to provide this. So why do scientists try to still look for life on these planets ? </p>

CC BY-SA 4.0
2018-11-21T23:51:27.577Z
How many books long should the answer be? I suggest to do a bit more prior research... a good start would be to google some "astrobiology" lectures online, there's always some free ones you can access legally.
AtmosphericPrisonEscape
CC BY-SA 4.0
2018-11-21T23:52:51.587Z
There are many living things that are not "like animals".
BowlOfRed
CC BY-SA 4.0
2018-11-22T00:28:58.790Z
Many organisms on Earth do not need oxygen to survive.
Anders Sandberg
CC BY-SA 4.0
2018-11-25T14:49:32.933Z
Welcome new user.  Just one thing - note that as a rule scientists are looking for evidence of *past life* on Mars, not so much life right now.
Fattie
<life>
Life on other planets
Dan Khan
# Life on other planets

(Asked by: username_0 on 2018-11-21)

If all living things like animals require oxygen to live, how can people think that there could be life on other planets such as mars for example ? Living things require oxygen and carbon dioxide, and these planets do not have plants and such to provide this. So why do scientists try to still look for life on these planets ?

**Tags:** life
> **Comments:**
> **username_1**: How many books long should the answer be? I suggest to do a bit more prior research... a good start would be to google some "astrobiology" lectures online, there's always some free ones you can access legally.  
> **username_2**: There are many living things that are not "like animals".  
> **username_3**: Many organisms on Earth do not need oxygen to survive.  
> **username_4**: Welcome new user.  Just one thing - note that as a rule scientists are looking for evidence of *past life* on Mars, not so much life right now.  

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## 2 answers

### Answer by username_5 on 2018-11-22. Score: 4 | Accepted answer

**TL;DR: Not all life requires atmospheric oxygen or carbon dioxide. There are many organisms here on Earth that use [chemosynthesis](https://en.wikipedia.org/wiki/Chemosynthesis) to process chemicals like methane or hydrogen sulphide for energy.**

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The search for life on Mars has concentrated on finding evidence of [autotrophic](https://en.wikipedia.org/wiki/Autotroph) microorganisms – organisms that convert simple chemicals in the environment into complex organic compounds. Most autotrophs use water as the reducing agent, but some can use other chemicals like hydrogen sulphide.

The energy source for these autotrophs can either be sunlight, in which case we call them [*phototrophs*](https://en.wikipedia.org/wiki/Phototroph) (which includes algae and green plants here on Earth), or obtained through the oxidation of electron donors in their environment, in which case they're called [*chemotrophs*](https://en.wikipedia.org/wiki/Chemotroph).

There's a wide variety of chemotrophs here on Earth, typically living in completely dark and often hostile environments such as next to deep-sea volcanic vents. For example, iron-oxidizing bacteria even colonise new lava beds in the deep ocean, and in effect use the oxidation of available ferrous iron as their respiratory process.

There's no reason to think that autotrophs couldn't find niche environments on Mars in which to exist, but the biggest hurdles are the significantly lower temperature and pressure, and the significantly greater radiation. The latter can be overcome by colonising *sub-surface* environments, which eliminates the phototrophs from contention. While UV radiation penetrates soils only in the millimetre range, [one study](http://discovery.ucl.ac.uk/134609/1/2006GL027494.pdf) found that viable dormant cells would have to be at least 7.5m below the planet's surface to survive the cumulative damage from cosmic radiation.


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### Answer by username_6 on 2018-11-22. Score: 1

What's more, in addition to finding potential evidence for life now, there is also the equally important possibility of past life that has gone extinct but left biosignatures like fossils or other geological byproducts. It is important to realize that there is considerable evidence that the Martian climate used to be very different, and there may have been a much denser atmosphere, providing the carbon dioxide that plant life would need to live on the surface and use photosynthesis. The fact that there is not a lot of oxygen in the atmosphere now suggests that there was not a multibillion year history of plant life like the Earth has (a lot of it without much oxygen), but there could have been a short period where life did thrive, and it might be hard to tell now that this ever happened-- without looking closely. But yes, it does seem likely that there are places in the galaxy more conducive to life than Mars, Mars is just the closest-- and you always start looking for your lost keys under the streetlights, going on only after you've eliminated that possibility.

> **Comments:**
> **username_5**: +1 for the additional detail! A denser atmosphere historically would address the problems with temperature and especially pressure (current pressure is too low for almost all cellular life), but I'm guessing would have a negligible impact on cosmic radiation, so I'm not sure that phototrophs would have been viable?  
> **username_6**: You mean the fact that Mars has little magnetic field to protect against energetic particles?  It might cause a lot of genetic damage, but would it sterilize the planet?  It is thought interaction with perchlorates might produce toxic surface compounds, so you may be right.  
> **username_5**: It's the cumulative genetic damage from energetic particles - see the link in last para of my post. The perchlorate problem is exacerbated by *UV* rather than energetic particles, and despite a quick search, I can't find if UV is absorbed by CO2. I'm assuming CO2 is only opaque to the longer IR wavelengths.  

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