Heavy Metal Frost? A New Look at a Venusian Mystery
|For Immediate Release|
|20 October 2014
GSA Release No. 14-75
Director of Education, Communication, & Outreach
during the meeting
19-22 Oct. 2014
Boulder, CO, USA — Venus is hiding something beneath its brilliant shroud of clouds: a first order mystery about the planet that researchers may be a little closer to solving because of a new re-analysis of twenty-year-old spacecraft data.
Venus's surface can't be seen from orbit in visible light because of the planet's hot, dense, cloudy atmosphere. Instead, radar has been used by spacecraft to penetrate the clouds and map out the surface – both by reflecting radar off the surface to measure elevation and by looking at the radio emissions of the hot surface. The last spacecraft to map Venus in this way was Magellan, two decades ago. One of the Venusian surprises discovered at that time is that radio waves are reflected differently at different elevations on Venus. Also observed were a handful of radio dark spots at the highest elevations. Both enigmas have defied explanation.
“There is general brightening upward trend in the highlands and then dark spots at the highest locations,” explained Elise Harrington, an Earth sciences undergraduate at Simon Fraser University, in British Columbia, who revisited the Venus data during her internship at the Lunar and Planetary Institute, under the direction of Allan Treiman. Brightening, in this case, means the radio waves reflect well. Dark means the radio waves are not reflected. In other words, the higher you go on Venus, the more radio reflective the ground gets until it abruptly goes radio black.
“Like on Earth, the temperature changes with elevation,” Harrington explained. And the cooler temperatures at altitude lead to ice and snow, which create a similar pattern of brightening for Earth – but in visible light. “Among the possibilities on Venus are a temperature dependent chemical weathering process or heavy metal compound precipitating from the air – a heavy metal frost.”
Getting to the bottom of these mysteries has been very hard because Venus has not been revisited since Magellan and no better data is available.
So Harrington and Trieman made do by re-purposing the old data. They used recently-available stereo radar elevation data (from Dr. R. Herrick, University of Alaska) rather than using the lower resolution radar altimetry. That increased their altimetry resolution from seeing patches 8 by 12 kilometers to just 600x600 meters. They also used Magellan's Synthetic Aperture Radar (SAR), with its 75x75-meter footprint, to look at radio reflectance, rather than the data on radio emissions from the surface, which had a coarser 15 by 23 kilometer resolution.
They applied these to two areas in the Odva Regio highlands region of Venus where they confirmed the same pattern of radar reflections brightening with increasing elevation, as was found by previous researchers. The radar reflection was low at the lower 2,400 meter (7,900 foot) elevation, then rapidly brightens up to 4,500 meters (14,700 feet). But they also found a lot more of those strange black spots, with a precipitous drop in the reflections at 4,700 meters (15,400 feet).
“The previous author saw a few dark spots,” said Harrington. “But we see hundreds of them.”
Years ago it was proposed that some sort of ferro-electric compound might be the cause of the brightening and the dark spots, but so far no specific compound has been identified which does the trick. Then again, with the surface of Venus being at almost 900 °F (500 °C) under more than 90 times the air pressure of Earth's atmosphere at sea level, with occasional showers of acid, it’s not easy to test the properties of materials under Venusian conditions.
“No one knows what explains the sudden darkness,” said Harrington, who will be presenting the work at the meeting of the Geological Society of America in Vancouver, B.C., on Monday, Oct. 20. “We think this might spur some more interest in Venus.”
THE PUZZLE OF RADAR-BRIGHT HIGHLANDS ON VENUS: A HIGH-SPATIAL RESOLUTION STUDY IN OVDA REGIO
[ Abstract ]
Session No. 136—Booth #266
T230. Topics in Planetary Geology (Posters)
HARRINGTON, Elise, Department of Earth Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC V5A 1S6, Canada
TREIMAN, Allan H., Lunar and Planetary Institute, 3600 Bay Area Blvd, Houston, TX 77058
Monday, 20 October 2014: 9:00 AM-6:30 PM
Vancouver Convention Centre-West Exhibition Hall C
PHOTO (click on image for high resolution version)
Caption: This is a radar image of one of the areas sampled on Ovda. There is a smooth ramp across the map going from higher to lower elevations, shown as a gradual transition in radar brightness up the ramp. (The top of the ramp is brighter than the bottom of the ramp in the lower right corner). The bright areas to either side of the ramp are highland plateaus, and the curious dark spots are the mysterious areas at the highest elevations that the researchers are investigating.
Additional image and information at http://www.lpi.usra.edu/vexag/reports/science_nuggets/2014_August_Treiman.pdf
The Geological Society of America, founded in 1888, is a scientific society with more than 26,500 members from academia, government, and industry in more than 100 countries. Through its meetings, publications, and programs, GSA enhances the professional growth of its members and promotes the geosciences in the service of humankind. Headquartered in Boulder, Colorado, GSA encourages cooperative research among earth, life, planetary, and social scientists, fosters public dialogue on geoscience issues, and supports all levels of earth science education.