Exploring Habitable Zones: Searching for Life Beyond Earth

In summary, there is still some uncertainty about whether or not liquid water exists on Mars, but it is a significant reason why we look for life there.
  • #1
cstoos
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With the confirmation of water on at least two other major bodies in our solar system so far (Mars, Moon), has this expanded the range of the "habitable zone" when searching for locations of possible life in the solar system?
 
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  • #2
The habitable zone is the range of distances from a sun where water is liquid.
water ice is present pretty much everywhere in the outer solar system - comets for instance are mostly ice
 
  • #3
Right, but we know that liquid water once flowed on Mars, correct?

There are also basic lifeform that survive in environments without water in it's liquid form so it seems to me that life could exist on the limits of the liquid water range...or even slightly past.

http://serc.carleton.edu/microbelife/extreme/withoutwater/
 
  • #4
cstoos said:
Right, but we know that liquid water once flowed on Mars, correct?
Not sure if that's totally accepted, water could have flowed as ice or as a hydrate, if there was liquid water it would only have existed while Mars had a much thicker atmosphere.

A bigger argument for a wider habitable zone is probably the moons of Jupiter, they can have liquid water ,below an ice covered surface, with the heat provided by tidal forces from jupiter.
 
  • #5
cstoos said:
Right, but we know that liquid water once flowed on Mars, correct?
From what I can gather, there's still a fair amount of uncertainty where this is concerned. See this blog post, for instance:
http://blogs.discovermagazine.com/b...5/are-martian-gullies-formed-by-water-or-not/

As near as I can tell, the evidence for liquid water on Mars largely consists of evidence from formations that we see on Mars that look very similar to formations on Earth which are, on Earth, formed only with water. However, as this paper shows, it is conceivable that other processes are producing these formations on Mars instead.

Regardless, the possibility of liquid water on Mars is one significant reason why probes we send there frequently look for life. We expect that if there is life on Mars, it would consist of a few hardy microbes.
 

Related to Exploring Habitable Zones: Searching for Life Beyond Earth

1. What is a habitable zone?

A habitable zone is the region around a star where it is possible for liquid water to exist on the surface of a planet.

2. How do we determine if a planet is in the habitable zone?

We can determine the habitable zone of a planet by looking at its distance from its star, the star's size and temperature, and the planet's atmospheric conditions.

3. What factors make a planet suitable for life?

A planet must have liquid water, a stable and suitable atmosphere, and a source of energy to be considered suitable for life. Other factors such as the planet's size, surface temperature, and geological activity may also play a role.

4. Are there other ways to search for life beyond Earth besides looking for habitable zones?

Yes, there are other methods such as searching for biosignatures, which are chemical or physical signs of life, or studying the atmospheric composition of planets to look for biomarkers.

5. Have we found any potentially habitable exoplanets?

Yes, scientists have discovered several exoplanets within the habitable zone of their stars, such as Proxima Centauri b and TRAPPIST-1e. However, more research is needed to determine if these planets are truly habitable.

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