Significant changes in Mars' atmosphere detected
NASA said today that its Mars Reconnaissance Orbiter found that the amount of the Red Planet's atmosphere depends on the tilt of its axis. And as the amount changes, so too could the stability of any liquid water on Mars.
NASA said today that new data from the(MRO) has demonstrated that the amount of atmosphere on the Red Planet depends entirely on the tilt of its axis. This is significant, the space agency said, because that axis tilt may well impact the stability of any liquid water that exists on Mars, as well as the frequency and strength of dust storms.
In a release, NASA explained that by employing the MRO's ground-penetrating radar, researchers were able to identify a massive subsurface deposit of frozen carbon dioxide--dry ice--on Mars' southern pole. "The scientists suspect that much of this carbon dioxide enters the planet's atmosphere and swells the atmosphere's mass when Mars' tilt increases," NASA reported.
With a volume of almost 3,000 cubic miles, the deposit contains 80 percent as much CO2 as that found in Mars' entire atmosphere. But so-called "collapse pits caused by dry ice sublimation and other clues suggest the deposit is in a dissipating phase," a process that puts more gas into the planet's atmosphere each year. By contrast, Mars' atmosphere is nearly 95 percent carbon dioxide, while Earth's has less than 0.04 percent of the substance.
NASA researchers said they had already been aware of a deposit of dry ice on top of liquid ice on Mars, but that the subsurface buildup contains about 30 times as much frozen carbon dioxide as was previously thought.
In addition, they said that at the moment, the planet's buildup of carbon dioxide is half frozen and half in its atmosphere, but that it can sometimes be almost entirely frozen or in the atmosphere--suggesting that as the planet rotates on its axis, the carbon dioxide shifts with it.
"An occasional increase in the atmosphere would strengthen winds, lofting more dust and leading to more frequent and more intense dust storms," NASA said in its release. "Another result is an expanded area on the planet's surface where liquid water could persist without boiling. Modeling based on known variation in the tilt of Mars' axis suggests several-fold changes in the total mass of the planet's atmosphere can happen on time frames of 100,000 years or less."
Ultimately, the effect of these changes can be dramatic. as Robert Haberle, a planetary scientist at NASA Ames' Research Center in Mountain View, Calif., put it in the release, if Mars is tilted on its axis and has an atmosphere thicker with carbon dioxide, a greenhouse effect is likely that attempts to heat up the surface of the planet. At the same time, if the polar ice caps are thicker and longer-lasting, a cooling effect is likely. "Our simulations show the polar caps cool more than the greenhouse warms," Haberle said in the release. "Unlike Earth, which has a thick, moist atmosphere that produces a strong greenhouse effect, Mars' atmosphere is too thin and dry to produce as strong a greenhouse effect as Earth's, even when you double its carbon-dioxide content."