Because planets either too close to or too far from their host stars will be at temperatures that cause water either to boil or to freeze, astrobiologists define a «habitable zone,» a range of orbital distances within which planets can
support liquid water on their surfaces.
In them a planet might still be able to
support liquid water on its surface if more exotic atmospheric compositions are allowed.
These planets in the habitable zones of their stars, while able to
support liquid water on their surfaces, develop in dry environments and need to have ice sent in from farther out.
In a paper published in Geophysical Research Letters, researchers found that interactions between methane, carbon dioxide and hydrogen in the early Martian atmosphere may have created warm periods when the planet could
support liquid water on the surface.
Because the stars are also faint, planets can be located close to the star and still have a temperature that
supports liquid water on the surface.
Not exact matches
Located 620 light - years away, it is the first planet found by NASA's Kepler space telescope to reside in its star's habitable zone — a region that can
support liquid water, a key requirement for life
on Earth.
«Here was a planet with all the elements needed to
support life in its atmosphere, with evidence of
liquid water in the past, and yet there was no life --[as if] Mars had the lights
on, but nobody was home,» he says.
It also offers among others an answer to the long - standing question of where the energy that can
support water in
liquid form
on the small, cryovulcanic moon far from the sun comes from.
She was suggesting that Europa's ocean was not its only source of
liquid water; the moon also harbored hidden lakes far closer to vital molecules
on the surface, perhaps close enough to
support miniature habitable ecosystems.
Climate models suggest the innermost planets, TRAPPIST - 1b, c and d, are probably too hot to
support liquid water, except maybe
on a small fraction of their surfaces.
All of the planet candidates are within the habitable zone, the orbital area that can
support the existence of
liquid water on the surface, and are considered Super-Earths.
The
liquid water habitable zone provides the best observational constraint
on where we would expect to find planets that could
support conscious observers like us, and this study examines the probability of finding oneself
on a planet in the habitable zone of a yellow dwarf star, compared to a red dwarf.
A world with an iron core, rocky mantle and enough
water on the surface to create
liquid water oceans that could
support life.
Since K2 - 18b is likely rocky, this means the planet could have
liquid water on its surface, which is one of many conditions for
supporting life.
Two of these planets, the researchers say, might barely be
on the edge of the habitable zone, that not - too - hot, not - too - cold region that can potentially
support liquid water and even life.
Of the 135 planets confirmed so far, only a few are thought to be in the habitable (or «Goldilocks») zone, where conditions
on the planet's surface can
support surface
liquid water.
If the models can accurately portray the Martian atmosphere billions of years ago, scientists might be able to answer critical questions like whether the atmosphere was once substantial enough to sustain
liquid water on its surface and
support life.
Clues
on the Martian surface, including features resembling dry riverbeds and minerals that only form in the presence of
water, suggest Mars once had a denser atmosphere that
supported the presence of
liquid water on the surface.
Four and a half billion years after its birth, the shrouded planet is much too hot to
support the presence of
liquid water on its surface because of its dense carbon dioxide atmosphere and sulfuric acid clouds, which retain too much radiative heat from the Sun through a runaway greenhouse effect.