Thursday, October 23, 2014

Could ‘Heavy Metal’ Frost Lurk Beneath Venus’ Hothouse Clouds?

Could ‘Heavy Metal’ Frost Lurk Beneath Venus’ Hothouse Clouds?:

A radar view of Venus taken by the Magellan spacecraft, with some gaps filled in by the Pioneer Venus orbiter. Credit: NASA/JPL

A radar view of Venus taken by the Magellan spacecraft, with some gaps filled in by the Pioneer Venus orbiter. Credit: NASA/JPL
Talk about using old data for a new purpose! Researchers re-examining information from the completed NASA Magellan mission found signs of what could be “heavy metal” frost on the hell-like surface. What the researchers saw in radio-wave reflectance is the highlands appear brighter, with dark spots in the tallest locations.

What substance exactly is causing the patches on the surface is unknown, and it is extremely hard to make predictions given the difficulty of simulating Venus’ 900-degree Fahrenheit (500-degree Celsius) surface temperature, which is also 90 times Earth’s air pressure at sea level.

“Like on Earth, the temperature changes with elevation,” stated Elise Harrington, an Earth sciences undergraduate at British Columbia’s Simon Fraser University who led the research. “Among the possibilities on Venus are a temperature dependent chemical-weathering process or heavy metal compound precipitating from the air – a heavy metal frost.”

Venus' volcano Sapas Mons, which was imaged by the Magellan mission in 1991. Credit: NASA


Venus’ volcano Sapas Mons, which was imaged by the Magellan mission in 1991. Credit: NASA
Scrutiny of a previously examined area on Venus, the Odva Regio highlands, saw a low radar reflection at 2,400 meters (7,900 feet), which progressively gets brighter until dark spots begin appearing and reflections drop at 4,700 meters (15,400 meters).

While previous research spotted a few of these patches, Harrington and supervisor Allan Treiman (Lunar and Planetary Institute) saw hundreds. There’s no radar-imaging spacecraft in orbit around Venus right now, but the authors hope that the finding will generate more interest in this planet. (Of note, the European Space Agency’s Venus Express is finishing up a mission there now, which included several daring atmosphere-skimming maneuvers earlier this year.)

The research was presented at the Geological Society of America meeting in Vancouver, British Columbia.

Source: Geological Society of America



About 

Elizabeth Howell is the senior writer at Universe Today. She also works for Space.com, Space Exploration Network, the NASA Lunar Science Institute, NASA Astrobiology Magazine and LiveScience, among others. Career highlights include watching three shuttle launches, and going on a two-week simulated Mars expedition in rural Utah. You can follow her on Twitter @howellspace or contact her at her website.

No comments:

Post a Comment