Jump to content

Ptolemaeus (Martian crater)

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Macrakis (talk | contribs) at 16:31, 31 December 2015 (it is "the" Ptolemy). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Template:MarsGeo-Crater Ptolemaeus Crater is a crater on Mars found in the Phaethontis quadrangle at 46.21° south latitude and 157.6° west longitude. It is 165.18 km in diameter and was named after Claudius Ptolemaeus (Ptolemy), the Greco-Egyptian astronomer (c. AD 90-160).[1] The Soviet probe Mars 3 is thought to have successfully landed in Ptolemaeus Crater in 1971, but contact was lost seconds after landing.[2] Mantle material that is believed to have fallen from the sky is visible in the crater.

  • Portion of Ptolemaeus Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Parts of the North and south rim are visible—at top and bottom of photo.
    Portion of Ptolemaeus Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Parts of the North and south rim are visible—at top and bottom of photo.

Ice-rich mantle

Much of the surface of Mars is covered by a thick smooth mantle that is thought to be a mixture of ice and dust.[3] This ice-rich mantle, a few yards thick, smoothes the land, but in places it has a bumpy texture, resembling the surface of a basketball. Under certain conditions the ice could melt and flow down the slopes to create gullies. Because there are few craters on this mantle, the mantle is relatively young. An excellent view of this mantle is shown below in the picture of the Ptolemaeus Crater Rim, as seen by HiRISE.

Changes in Mars's orbit and tilt cause significant changes in the distribution of water ice from polar regions down to latitudes equivalent to Texas. During certain climate periods water vapor leaves polar ice and enters the atmosphere. The water comes back to ground at lower latitudes as deposits of frost or snow mixed generously with dust. The atmosphere of Mars contains a great deal of fine dust particles. Water vapor will condense on the particles, then fall down to the ground due to the additional weight of the water coating. When ice at the top of the mantling layer goes back into the atmosphere, it leaves behind dust, which insulating the remaining ice.[4]

  • This topographic map shows volcanic peaks in white because of their great height. Near the equator, a line of three volcanoes points south to Phaethontis and three large craters-the area where there are many gullies. Click on the image for a good view.
    This topographic map shows volcanic peaks in white because of their great height. Near the equator, a line of three volcanoes points south to Phaethontis and three large craters-the area where there are many gullies. Click on the image for a good view.
  • Ptolemaeus Crater Rim, as seen by HiRISE. Click on image to see excellent view of mantle deposit.
    Ptolemaeus Crater Rim, as seen by HiRISE. Click on image to see excellent view of mantle deposit.

References

  1. ^ "Ptolemaeus (Martian crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^ Lakadawalla, Emily. "Russia's Mars 3 lander maybe found by Russian amateurs". The Planetary Society. Retrieved 20 January 2014.
  3. ^ Head, J. et al. 2003. Recent ice ages on Mars. Nature:426. 797-802.
  4. ^ MLA NASA/Jet Propulsion Laboratory (2003, December 18). Mars May Be Emerging From An Ice Age. ScienceDaily. Retrieved February 19, 2009, from http://www.sciencedaily.com /releases/2003/12/031218075443.htmAds by GoogleAdvertise

See also


Stub icon

This article about the planet Mars or its moons is a stub. You can help Wikipedia by expanding it.

Stub icon

This article about an extraterrestrial geological feature is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Ptolemaeus_(Martian_crater)&oldid=697607979"