Subscribe free to our newsletters via your
  Mars Exploration News  

Subscribe free to our newsletters via your

Frosty Cold Nights Year-Round on Mars May Stir Dust
by Staff Writers
Pasadena CA (JPL) Jul 12, 2016

This map shows the frequency of carbon dioxide frost's presence at sunrise on Mars, as a percentage of days year-round. Carbon dioxide ice more often covers the ground at night in some mid-latitude regions than in polar regions, where it is generally absent for much of summer and fall. Image courtesy NASA/JPL-Caltech. For a larger version of this image please go here.

Some dusty parts of Mars get as cold at night year-round as the planet's poles do in winter, even regions near the equator in summer, according to new NASA findings based on Mars Reconnaissance Orbiter observations.

The surface in these regions becomes so frigid overnight that an extremely thin layer of carbon dioxide frost appears to form. The frost then vaporizes in the morning. Enough dust covers these regions that their heat-holding capacity is low and so the daily temperature swing is large. Daily volatilization of frost crystals that form among the dust grains may help keep the dust fluffy and so sustain this deep overnight chill.

Carbon dioxide is the main ingredient of Mars' atmosphere. The planet also has large reserves of frozen carbon dioxide buried in the polar ice caps. Seasonal buildup and thawing of carbon dioxide frost at high latitudes on Mars have been studied for years and linked to strange phenomena such as geyser-like eruptions and groove-cutting ice sleds.

Here's what's new knowledge: the presence and extent of transient overnight carbon dioxide frosts, even at middle and low latitudes. Infrared-wavelength observations of dust-covered regions by the Mars Climate Sounder instrument on NASA's Mars Reconnaisance Orbiter not only indicate cold-enough nighttime surface temperatures for carbon dioxide frost to form, they also detect a spectrum signature at night consistent with a trace of frost.

"The temperature gets so low, you start freezing the atmosphere onto the surface," said Sylvain Piqueux of NASA's Jet Propulsion Laboratory, Pasadena, California, lead author of a report on these findings published online by the Journal of Geophysical Research: Planets. "Once you reach that temperature, you don't get colder, you just accumulate more frost. So even on the polar caps, the surface temperature isn't any colder than what these lower-latitude regions get to overnight."

Three middle- and low-latitude areas in the Tharsis, Arabia and Elysium regions of Mars have nightly temperatures cold enough for carbon dioxide frost year-round or nearly year-round. Each of the three is bigger than Texas. All three are dust-covered to the extent that surface temperatures change much quicker than in areas with exposed-bedrock surfaces.

Piqueux said, "These same regions that are coldest at night are the warmest during the day. It has to do with the nature of the material - it's so fluffy. Think of when you're at the beach on a summer afternoon, where you step on the fine grain sand. You almost burn your foot, it's so hot at the surface, but just below the surface it's not as hot, and if you touch a boulder, it doesn't feel as hot. Then it's the opposite at night: The surface of the sand cools off quickly, while the boulder stays warm."

Unlike the polar regions, at lower latitudes the atmosphere is warmer than the ground at night. A critical step in understanding just how cold the ground in these areas gets at night was correcting observations of the planet's surface for slightly warmer atmospheric temperatures. Temperatures are determined from orbit by analyzing the infrared radiation oserved at the top of the atmosphere; this includes radiation from both the ground and the atmosphere. The Mars Climate Sounder instrument, by observing both sideways toward the horizon from orbit and downward, can record infrared emissions from a cross-section of the atmosphere, as well as from the planet's surface. Analysis then reveals the true - colder - ground temperature.

The same instrument also provides readings at multiple infrared wavelengths, yielding results consistent with the presence of microscopic-scale carbon dioxide frost crystals forming a layer no thicker than a few sheets of paper.

"If at night you form little frost crystals between the grains of dust on the surface, pushing the grains apart, then the frost crystal becomes a little puff of air in the morning, that might be helping to maintain the fluffiness of the surface," Piqueux said. "You prevent the cementation of grains, the locking together of grains into a more consolidated surface. It's a self-maintaining process: Where you keep the soil fluffy, you maintain the conditions to form frost at night."

"A cycle of carbon dioxide frost that happens every night could be related to other active processes on Mars," said Rich Zurek, JPL's chief Mars scientist. "This agitation of the soil would affect surface physical properties and could have implications for erosive processes and for the exchange of water vapor between the atmosphere and surface."

Many streaks on Martian slopes appear to be slides of dry material, with no liquid involved. The lubrication effect of carbon dioxide frost thawing directly into gas has been linked to such slides where winter frost thaws in spring. Daily frost cycles may have similar effects.

Another type of slope activity on Mars is called recurring slope lineae (RSL). These appear as dark streaks advancing downhill in a warm season, then fade away, then re-appear the next warm season. Hydrated salt has been confirmed at some of these sites, and they are considered the strongest evidence for the possible presence of liquid water on the surface of modern Mars. "Although RSL appear to start on steep, rocky slopes, the realization that overnight carbon dioxide frosts occur even during warm seasons adds another factor to be considered in RSL activity," Zurek said.

The science instruments on NASA's Mars Reconnaissance Orbiter have been examining Mars since 2006. JPL, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate in Washington and built the Mars Climate Sounder. Lockheed Martin Space Systems of Denver built the orbiter and supports its operations.

Research paper: "Discovery of a widespread low-latitude diurnal CO2 frost cycle on Mars"

Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Contributor
$5 Billed Once

credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly

paypal only


Related Links
Mars Reconnaissance Orbiter
Mars News and Information at
Lunar Dreams and more

Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks DiggDigg RedditReddit GoogleGoogle

Previous Report
ChemCam findings hint at oxygen-rich past on Mars
Los Alamos NM (SPX) Jul 01, 2016
The discovery of manganese oxides in Martian rocks might tell us that the Red Planet was once more Earth-like than previously believed. A new paper in Geophysical Research Letters reveals that NASA's Curiosity rover observed high levels of manganese oxides in Martian rocks, which could indicate that higher levels of atmospheric oxygen once existed on our neighboring planet. This hint of mo ... read more

Russia to spend $60M in 2016-2018 to fund space voyages to Moon, Mars

Russian Moon Base to Hold Up to 12 People

US may approve private venture moon mission: report

Fifty Years of Moon Dust

Dutch Radio Antenna to Depart for Moon on Chinese Mission

Chinese Space Garbageman is not a Weapon

China to launch its largest carrier rocket later this year

China committed to peaceful use of outer space

New Crew Members, Including NASA Biologist, Launch to Space Station

Three astronauts blast off for ISS in upgraded Soyuz craft

Soyuz-FG to launch new crew to ISS fully assembled

Down to Earth: Returned astronaut relishes little things

New Horizons Receives Mission Extension to the Kuiper Belt

Alex Parker Discovers Moon Over Makemake in the Kuiper Belt

Hubble locates new dark spot on Neptune

Pluto's Subsurface Ocean Likely Exists Today

Chemical Trail Could Lead To Clues About Life On Titan

Chemical trail on Titan may be key to prebiotic conditions

An Ocean Lies a Few Kilometers Beneath Enceladus's Icy Surface

Cassini goes up and over for final mission tour of Saturn

SIIS started KOMPSAT-3A commercial services

Vision through the clouds

Experts call for satellite tech to be used in Africa's anti-poaching efforts

Sentinel-1 satellites combine radar vision

Mathematical framework prioritizes key patterns to accelerate scientific discovery

A decade of plant biology in space

Exploring inner space for outer space

Quantum technologies to revolutionize 21st century

Lush Venus? Searing Earth? It could have happened

A surprising planet with three suns

Teenagers at Keele University Discover Possible New Exoplanet

What Happens When You Steam a Planet

Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News

The content herein, unless otherwise known to be public domain, are Copyright 1995-2017 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement