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Emily LakdawallaJune 18, 2015

Transient hot spots on Venus: Best evidence yet for active volcanism

In a paper released in Geophysical Research Letters today, Eugene Shalygin and coauthors have announced the best evidence yet for current, active volcanism on Venus. The evidence comes from the Venus Monitoring Camera, which saw transient hot spots in four locations along a system of rifts near Venus' equator. They saw the hot spots in two distinct episodes in 2008 and 2009.

The press release describes the science pretty well, so I won't belabor that here; I thought I'd show you some pretty pictures of the region, made from Magellan data. Magellan obtained radar images of more than 97% of the planet, which have been merged into several enormous global data sets. To get the best-quality Magellan data you have to interact with an extremely klunky interface through the USGS, but it's well worth the effort. Here is the region in which Shalygin et al. report observing the hot spots. Click through twice to see it at its glorious full resolution. (Warning: 13 MB!)

Ganis chasmata, Venus: Site of active volcanism?

NASA / JPL / Emily Lakdawalla

Ganis chasmata, Venus: Site of active volcanism?
In 2008 and 2009, Venus Express saw transient hot spots in this region of Venus, a site near the equator called Ganis Chasma. There are enormous volcanoes in this area (Ozza Mons at lower right and Maat Mons at lower left) but the hot spots were along the fissures that cross the image from upper left to lower right. The whole region visible here is about 2000 kilometers square. This image is made from data from the Magellan mission, which ended in 1994.

Here, I've annotated the image with names of craters (yellow), mountains and chasmata (lighter and darker red), plains (blue), and the areas in which VMC saw hot spots (white).

Ganis chasmata, Venus: Site of active volcanism? (annotated)

These areas were imaged hundreds of times by VMC, but the hot spots only appeared very briefly. Crucially, two of the hot spots appeared in more than one orbit right after the other -- so it wasn't just one spurious detection. From the supplemental information to the paper, here's what we know about the hot spots:

These are not quite "liquid hot magma" temperatures, but they're very close. If VMC was seeing the cooling surface of a lava flow, those temperatures would be very reasonable.

In making the map, I noticed that the paper seems to have a nomenclature error: they talk about "Ganiki Chasma," but they're actually talking about Ganis Chasma; its name has been confused for nearby Ganiki Planitia. (Ganis Chasma was named for a western Lapp forest maiden, while Ganiki Planitia was named for a Siberian water spirit.)

Do enlarge the top image by clicking through it twice to enjoy the beautiful diversity of the Venusian landscape. This area has it all: small shield volcanoes and gigantic volcanic constructs; wide spreading lava flows; impact craters, some of them filled by lava; a particularly fresh impact crater (Sitwell) with a dark parabola; and that system of fissures. Here is one zoom in on the region containing Shalygin's Objects A and D. I feel like I can almost make out landslides running down the chasm walls here. Magellan image resolution is always just short of what I really want to see the features I'm interested in.

Ganis chasmata, Venus: Site of active volcanism? (detail)

NASA / JPL / Emily Lakdawalla

Ganis chasmata, Venus: Site of active volcanism? (detail)

If those hot spots are fresh lava flows, whence did they emanate? Did lava fill any of these chasms? If we were to return a radar mission to Venus, would this area have visible changes? There's only one way to find out. Let's go back to Venus!

Read more: pretty pictures, Venus missions before 2000, Venus Express, Venus, geology, explaining science

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Emily Lakdawalla

Solar System Specialist for The Planetary Society
Read more articles by Emily Lakdawalla

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