United kingdom Daily news: What does a Martian snowstorm look like? Researchers solve the puzzle and find that carbon dioxide 'snowflakes' are the size of a blood cell

What does a Martian snowstorm look like? Researchers solve the puzzle and find that carbon dioxide 'snowflakes' are the size of a blood cell

By Eddie Wrenn

PUBLISHED: 07:26 EST, 20 June 2012 | UPDATED: 07:26 EST, 20 June 2012

In the dead of a Martian winter, clouds of snow blanket the desolate Red Planetâ€™s poles.

But unlike our water-based snow, the particles on Mars are frozen crystals of carbon dioxide.

Most of the Martian atmosphere is composed of carbon dioxide, and in the winter, the poles get so cold - cold enough to freeze alcohol - that the gas condenses, forming tiny particles of snow.

Now researchers at MIT have calculated the size of snow particles in clouds at both Martian poles from data gathered by orbiting spacecraft.

From their calculations, the group found snow particles in the south are slightly smaller than snow in the north - but either way, the particles at both poles are small - about the size of a red blood cell.

Floating through the void, Mars sits in peace, although with a light fluttering of 'snow' at the poles, as shown in this artist's impression

Kerri Cahoy, the Boeing career development assistant professor of Aeronautics and Astronautics at MI, said: 'These are very fine particles, not big flakes.

'You would probably see it as a fog, because theyâ€™re so small.'

Cahoy and graduate student Renyu Hu, along with Professor Maria Zuber analysed libraries of data gathered from instruments onboard the Mars Global Surveyor (MGS) and Mars Reconnaissance Orbiter (MRO).

From the data, they determined the size of carbon dioxide snow particles in clouds, using measurements of the maximum buildup of surface snow at both poles.

The buildup is about 50 percent larger at Marsâ€™ south pole than its north pole.

Over the course of a Martian year (a protracted 687 days, versus Earthâ€™s 365), the researchers observed that as it gets colder and darker from fall to winter, snow clouds expand from the planetâ€™s poles toward its equator.

The snow reaches halfway to the equator before shr inking back toward the poles as winter turns to spring, much like on Earth.

'For the first time, using only spacecraft data, we really revealed this phenomenon on Mars,' says Hu, lead author of a paper published in the Journal of Geophysical Research, which details the groupâ€™s results.

Snow on Mars: The surface of the planet, littered with crater holes, may occasionally get a dusting of 'snow' at the poles

FINDING THE SIZE OF A SNOWFLAKE: HOW HU'S TEAM SOLVED THE PUZZLE

To get an accurate picture of carbon dioxide condensation on Mars, Hu analyzed an immense amount of data, including temperature and pressure profiles taken by the MRO every 30 seconds over the course of five Martian years (more than nine years on Earth).

The researchers looked through the data to see where and when conditions would allow carbon dioxide cloud particles to form.

The team also sifted through measurements from the MGSâ€™ laser altimeter, which measured the topography of the planet by sending laser pulses to the surface, then timing how long it took for the beams to bounce back.

Every once in a while, the instrument picked up a strange signal when the beam bounced back faster than anticipated, reflecting off an anomalously high point above the planetâ€™s surface. Scientists figured these laser beams had encountered clouds in the atmosphere.

Hu analysed these cloud returns, looking for additional evidence to confirm carbon dioxide condensation.

He looked at every case where a cloud was detected, then tried to match the laser altimeter data with concurrent data on local temperature and pressure.

In 11 instances, the laser altimeter detected clouds when temperature and pressure conditions were ripe for carbon dioxide to condense.

Hu then analysed the opacity of each cloud - the amount of light reflected - and through calculations, determined the density of carbon dioxide in each cloud.

To estimate the total mass of carbon dioxide snow deposited at both poles, Hu used earlier measurements of seasonal variations in the Martian gravitational field done by Zuberâ€™s group.

As snow piles up at Marsâ€™ poles each winter, the planetâ€™s gravitational field changes by a tiny amount.

By analysing the gravitational difference through the seasons, the researchers determined the total mass of snow at the north and south poles.

Using the total mass, Hu figured out the number of snow particles in a given volume of snow cover, and from that, determined the size of the particles.

In the north, molecules of condensed carbon dioxide ranged from 8 to 22 microns, while particles in the south were a smaller 4 to 13 microns.

'Itâ€™s neat to think that weâ€™ve had spacecraft on or around Mars for over 10 years, and we have all these great datasets.

''If you put different pieces of them together, you can learn something new just from the data.'

Since carbon dioxide makes up most of the Martian climate, understanding how it behaves on the planet will help scientists understand Marsâ€™ overall climate, says Paul Hayne, a postdoc in planetary sciences at the California Institute of Technology.

'The big-picture question this addresses is how the seasonal ice caps on Mars form,' says Hayne, who was not involved in the research.

'The ice could be freezing directly at the surface, or forming as snow particles in the atmosphere and snowing down on the surface â€¦ this work seems to show that at least in some cases itâ€™s snowfal l rather than direct ice deposition. Thatâ€™s been suspected for a long time, but this may be the strongest evidence.'

Hayne said knowing the size of carbon dioxide snow cloud particles on Mars may help researchers understand the properties and behavior of dust in the planetâ€™s atmosphere.

For snow to form, carbon dioxide requires something around which to condense - for instance, a small silicate or dust particle. 'What kinds of dust do you need to have this kind of condensation?' Hu asks. 'Do you need tiny dust particles? Do you need a water coating around that dust to facilitate cloud formation?'

Just as snow on Earth affects the way heat is distributed around the planet, Hu says snow particles on Mars may have a similar effect, reflecting sunlight in various ways, depending on the size of each particle.