The Tader Valles are a set of small channels in the Phaethontis quadrangle found at 49.1° south latitude and 152.5° west longitude. They are named after the ancient name for present Segura River, Spain.

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. This ice-rich mantle, a few yards thick, smooths 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. This mantle probably fills the Tader Valles as shown in the HiRISE image below. 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 insulates the remaining ice.MLA NASA/Jet Propulsion Laboratory (2003, December 18). Mars May Be Emerging From An Ice Age. ScienceDaily. Retrieved February 19, 2009, from https://www.sciencedaily.com/releases/2003/12/031218075443.htmAds by GoogleAdvertise Image:Phaethontis.JPG, Map of Phaethontis quadrangle. Click on to enlarge and see some crater names. Image:Tader Valles.JPG, The Tader Valles, as seen by THEMIS. Smooth material in channels may be a mantle in the form of dirty snow.

References

{{Portal bar, Solar System Phaethontis quadrangle Valleys and canyons on Mars

Ice-rich mantle

See also

References