Hellas Planitia - Video Learning - WizScience.com
"
Hellas Planitia" is a plain located within the huge, roughly circular impact basin Hellas located in the southern hemisphere of the planet
Mars. Hellas is the second or third largest impact crater and the largest visible impact crater known in the
Solar System.
The basin floor is about 7152 m deep,
3000 m deeper than the
Moon's
South Pole-Aitken basin, and extends about
2300 km east to west. It is centered at Hellas Planitia is in the
Hellas quadrangle and the
Noachis quadrangle.
With a diameter of about 2300 km, it is the largest unambiguous impact structure on the planet, though a distant second if the
Borealis Basin proves to be an impact crater. Hellas Planitia is thought to have been formed during the
Late Heavy Bombardment period of the Solar System, approximately 4.1 to 3.8 billion years ago, when a large asteroid hit the surface.
The altitude
difference between the rim and the bottom is 9000 m. The depth of the crater below the standard topographic datum of Mars) explains the atmospheric pressure at the bottom: 12.4 mbar during the northern summer
. This is 103% higher than the pressure at the topographical datum and above the triple
point of water, suggesting that the liquid phase could be present under certain conditions of temperature, pressure, and dissolved salt content. It has been theorized that a combination of glacial action and explosive boiling may be responsible for gully features in the crater.
Some of the low elevation outflow channels extend into Hellas from the volcanic
Hadriacus Mons complex to the northeast, two of which
Mars Orbiter Camera images show contain gullies:
Dao Vallis and
Reull Vallis. These gullies are also low enough for liquid water to be transient around
Martian noon, if the temperature would rise above 0
Celsius.
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The Place Inside" by
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Hellas+Planitia, which is released under
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