Carbon Dioxide Snow Storms During the Polar Night on Mars
The Mars Orbiter Laser Altimeter (MOLA) detected clouds associated with topographic features during the polar night on Mars. While uplift generated from flow over mountains initiates clouds on both Earth and Mars, we suggest that the Martian clouds differ greatly from terrestrial mountain wave cloud...
Main Authors: | , |
---|---|
Language: | unknown |
Published: |
2001
|
Subjects: | |
Online Access: | http://hdl.handle.net/2060/20010038655 |
id |
ftnasantrs:oai:casi.ntrs.nasa.gov:20010038655 |
---|---|
record_format |
openpolar |
spelling |
ftnasantrs:oai:casi.ntrs.nasa.gov:20010038655 2023-05-15T18:02:12+02:00 Carbon Dioxide Snow Storms During the Polar Night on Mars Toon, Owen B. Colaprete, Anthony Unclassified, Unlimited, Publicly available [2001] application/pdf http://hdl.handle.net/2060/20010038655 unknown Document ID: 20010038655 http://hdl.handle.net/2060/20010038655 No Copyright CASI Lunar and Planetary Science and Exploration 2001 ftnasantrs 2019-07-21T07:53:31Z The Mars Orbiter Laser Altimeter (MOLA) detected clouds associated with topographic features during the polar night on Mars. While uplift generated from flow over mountains initiates clouds on both Earth and Mars, we suggest that the Martian clouds differ greatly from terrestrial mountain wave clouds. Terrestrial wave clouds are generally compact features with sharp edges due to the relatively small particles in them. However, we find that the large mass of condensible carbon dioxide on Mars leads to clouds with snow tails that may extend many kilometers down wind from the mountain and even reach the surface. Both the observations and the simulations suggest substantial carbon dioxide snow precipitation in association with the underlying topography. This precipitation deposits CO2, dust and water ice to the polar caps, and may lead to propagating geologic features in the Martian polar regions. Other/Unknown Material polar night NASA Technical Reports Server (NTRS) |
institution |
Open Polar |
collection |
NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
language |
unknown |
topic |
Lunar and Planetary Science and Exploration |
spellingShingle |
Lunar and Planetary Science and Exploration Toon, Owen B. Colaprete, Anthony Carbon Dioxide Snow Storms During the Polar Night on Mars |
topic_facet |
Lunar and Planetary Science and Exploration |
description |
The Mars Orbiter Laser Altimeter (MOLA) detected clouds associated with topographic features during the polar night on Mars. While uplift generated from flow over mountains initiates clouds on both Earth and Mars, we suggest that the Martian clouds differ greatly from terrestrial mountain wave clouds. Terrestrial wave clouds are generally compact features with sharp edges due to the relatively small particles in them. However, we find that the large mass of condensible carbon dioxide on Mars leads to clouds with snow tails that may extend many kilometers down wind from the mountain and even reach the surface. Both the observations and the simulations suggest substantial carbon dioxide snow precipitation in association with the underlying topography. This precipitation deposits CO2, dust and water ice to the polar caps, and may lead to propagating geologic features in the Martian polar regions. |
author |
Toon, Owen B. Colaprete, Anthony |
author_facet |
Toon, Owen B. Colaprete, Anthony |
author_sort |
Toon, Owen B. |
title |
Carbon Dioxide Snow Storms During the Polar Night on Mars |
title_short |
Carbon Dioxide Snow Storms During the Polar Night on Mars |
title_full |
Carbon Dioxide Snow Storms During the Polar Night on Mars |
title_fullStr |
Carbon Dioxide Snow Storms During the Polar Night on Mars |
title_full_unstemmed |
Carbon Dioxide Snow Storms During the Polar Night on Mars |
title_sort |
carbon dioxide snow storms during the polar night on mars |
publishDate |
2001 |
url |
http://hdl.handle.net/2060/20010038655 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
polar night |
genre_facet |
polar night |
op_source |
CASI |
op_relation |
Document ID: 20010038655 http://hdl.handle.net/2060/20010038655 |
op_rights |
No Copyright |
_version_ |
1766171990363734016 |