See other posts from January 2012
Is there life on Venus? Not in reprocessed Venera-13 images.
Posted by Emily Lakdawalla
2012/01/23 12:56 CST
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At the end of last week, a rather sensational article appeared in both the Russian- and English-language sites of the Russian news agency, RIA Novosti. "Life Spotted on Venus - Russian Scientist," ran the English headline; a Google translation of the Russian one goes: "The Soviet probes may have photographed creatures on Venus." Accompanying the article are photos from the Venera-13 lander, one blown up to a rather ridiculous extent, with a blob circled, labeled "Scorpion."
The story is so obviously ridiculous that I would ordinarily not give it a second thought. But one thing gave me pause, and that's the author. Leonid Ksanfomaliti is a senior statesman of Russian planetary science. In addition to his scientific and technical contributions, he is also a popularizer, a speaker and writer who brings space science to the public.
Leonid Ksanfomaliti
Biography from Don Mitchell's website: L.V. Ksanfomaliti graduated from the Leningrad Technical University in 1956, and after working at the Abastumani Observatory, he joined the Space Research Institute (IKI) in 1968. He is Chief of the Laboratory on Photometry and Thermal Radiometry. Mars-3 to Mars-7 included thermal, visual and ultraviolet radiometers of his design. During the Venera-9 and 10 mission, he worked on infrared and ultraviolet spectroscopy and imaging, helping to analyze the structure and dynamics of the Venusian clouds. His famous GROZA sensors on Venera-11 to Venera-14 were the first devices to detect intense lightning storms on Venus. Ksanfomaliti has continued his work on infrared spectroscopy and the study of cometary dust, with the Vega mission to Halley's comet and the 1988 Fobos mission to Mars. Recent work has included study of water and possibilities of life on Mars, and a new Earth-based imaging technique has produced images of unseen portions of the surface of Mercury.Before I continue, let's review briefly this decade of Venus exploration. Beginning with Venera 8, in 1972, the Soviet Union landed successfully on Venus nine times. All but the first of the Venera landers was accompanied by an orbiter for data relay. In most cases, the landers were still functioning when the orbiters passed out of range. The orbiters also performed their own remote sensing science. There's a detailed history and summary of the science results of these missions on Don Mitchell's website, in two parts (Venera-8 through -10 and Venera-11 through -14). Although the last Venera landing was 30 years ago, in 1982, the data from these missions continue to be the only "ground truth" we have for all the orbital, flyby, and Earth-based exploration that's been done since. Following the seven Venera landers, two Vega balloon probes landed in 1985, on the night side of Venus, after floating downward for nearly two days.
| Mission | Panoramic hotos? | Launched | Landed | Surface ifetime |
|---|---|---|---|---|
| Venera 8 | no | March 27, 1972 | July 22, 1972 | 50 min |
| Venera 9 | yes | June 8, 1975 | October 22, 1975 | 53 min |
| Venera 10 | yes | June 14, 1975 | October 25, 1975 | 65 min |
| Venera 11 | no | September 9, 1978 | December 25, 1978 | 95 min |
| Venera 12 | no | September 14, 1978 | December 21, 1978 | 110 min |
| Venera 13 | yes | October 30, 1981 | March 1, 1982 | 127 min |
| Venera 14 | yes | November 4, 1981 | March 5, 1982 | 57 min |
| Vega 1 | no | December 15, 1984 | June 11, 1985 | 20 min |
| Vega 2 | no | December 21, 1984 | June 15, 1985 | 20 min |
etting back to Ksanfomaliti's article. He says that it is worth re-examining the Venera lander images in particular. His reasoning: to date, most analyses of the photos have been based on a single panorama from each site. These published panoramas are, in fact, mosaics. Most of the landers took and transmitted several photos with each camera, several back-and-forth swings. All of them suffered from some loss of data to noise or other transmission problems, so the published panoramas are composed of the best parts of each of the panoramas. In the present paper, Ksanfomaliti takes the panoramas separately and examines them to see if there are noticeable changes from one frame to the next. Then, he says, we can attempt to discern whether these changes are related to abiological phenomena (such as wind) or whether they are related to his proposal that the planet is inhabited. Also, he says, by examining their shape, we can distinguish whether they have the "ordinary form of surface detail," or whether they look extraordinary.
This is, for me, where the paper begins to run off the rails. It's an excellent notion to examine successive panoramas to look for surface changes. In fact, it's been done before, and it's clear that surface changes did take place from one panorama to the next. Don Mitchell writes on his website about Venera-13 images: "Two images, taken about an hour apart, show the gradual blowing away of soil on the landing ring of Venera-13. Changes in the quality of illumination appear, becoming less diffuse at some times. This is probably due to the movement of clouds, which would probably cause vague regions of lighter and darker sky as seen from the surface." It's very important to recall that the sites that the Venera landers photographed -- actually, sites photographed by any lander of any planet -- are at least somewhat disturbed by the landing. The Veneras kicked up dust and soil that was redeposited on their flat surfaces, some of which was blown away in the brief period that they transmitted data to the surface.
There's another reason that successive images may look different, and that has to do with how they were transmitted to Earth. They were sent using two different types of modulation of the orbiter's carrier signal. The different types of modulation produced different kinds of noise. It's interesting to compare two of the Venera-13 photos' pixel values, as Don Mitchell has done in the graph below. If the two photos were identical, this graph would contain a single line at a 45-degree angle. Data dropouts result in gaps in this line (the value in one of the two images is zero). If the two photos were identical except for one or two tiny objects that moved, it would be a single line with a couple of very small, localized deviations. What we have instead is two photos that are fundamentally similar (most points cluster near that 45-degree line), but where there is a spread to the 45-degree line, indicating a distribution of pixel values around the expected ones. On top, there are some odd systematic variations in a few spots in the photo. There are, in fact, a lot of differences between the two photos, but it's almost all noise.
![]() Comparing two versions of Venera-13 panoramas This graph is a comparison of the pixel values in one of the Venera-13 panoramic images to the values of the same pixels in another one transmitted later. The two images were transmitted to Earth using different methods of modulating the radio signal, one pulse-code and the other pulse-time modulated. Credit: Don Mitchell |
![]() A processed Venera-13 view of Venus Credit: L. Ksanfomaliti, Solar System Research |
![]() "Changes" in successive Venera-13 images Credit: L. Ksanfomaliti, Solar System Research |
It's surprising that someone so otherwise respectable can publish something so patently off the wall. As I've chatted with people, various explanations have come up. One person told me that Ksanfomaliti has always had a penchant for things slightly on the edge of reality. Another suggests that thirty years of poring over old data sets, with no successful planetary missions producing new data sets, would make anyone crazy. As for me, I've seen before when successful people become so convinced that they are smart and right that they go over some edge and suddenly think that any crazy idea that flits into their head must be right, because they thought it and they're always right, right? There's no way for me to know what's made Ksanfomaliti make so much out of absolutely nothing. All I know is, there's nothing here. Move along.
And let's send another mission to land on Venus so we can finally get some new data already! Or maybe a long-lived Venus balloon!
![]() Prototype Venus Balloon Scientists hope to use a balloon such as this one, 9 meters in diameter, to study the atmosphere of Venus from below its clouds. A helium-filled Teflon balloon could stay high enough above the ground (at an altitude of about 56 kilometers) to avoid cooking at Venus' high surface temperatures, and would be resistant to corrosion from the sulfuric acid in Venus' clouds. Credit: NASA / JPL |
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