Visit NASA's Home Page Jet Propulsion Laboratory California Institute of Technology View the NASA Portal Click to search JPL Visit JPL Home Page Proceed to JPL's Earth Page Proceed to JPL's Solar System Page Proceed to JPL's Stars & Galaxies Page Proceed to JPL's Technology Page Proceed to JPL's People and Facilities Photojournal Home Page View the Photojournal Image Gallery
Top navigation bar

PIA00307: Perspective View of Venus (Center Latitude 45 Degrees N., Center Longitude 11 Degrees E.)
Target Name: Venus
Is a satellite of: Sol (our sun)
Mission: Magellan
Spacecraft: Magellan
Instrument: Imaging Radar
Product Size: 2000 samples x 1600 lines
Produced By: U.S. Geological Survey
Addition Date: 1998-06-04
Primary Data Set: Magellan MIDRs
Full-Res TIFF: PIA00307.tif (4.943 MB)
Full-Res JPEG: PIA00307.jpg (693.5 kB)

Click on the image to download a moderately sized image in JPEG format (possibly reduced in size from original).

Original Caption Released with Image:
This perspective view of Venus, generated by computer from Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia. Circular depressions with associated fracture patterns called "coronae" are apparently unique to the lowlands of Venus, and tend to occur in linear clusters along the planet's major tectonic belts. Coronae differ greatly in size and detailed morphology: the central depression may or may not lie below the surrounding plains, and may or may not be surrounded by a raised rim or a moat outside the rim. The corona shown here is relatively small (~100 km in diameter and ~1 km deep) and is of the subtype known as an "arachnoid" because of the spider-like configuration of concentric (body) and radial (legs) fractures. Coronae are thought to be caused by localized "hot spot" magmatic activity in Venus' subsurface. Intrusion of magma into the crust first pushes up the surface, after which cooling and contraction create the central depression and generate a pattern of concentric fractures. In some cases, lava may be extruded onto the surface. The fractured ridge at the left is classified as a "nova" or "stellate fracture center" and is believed to represent an early phase of corona formation, in which subsidence due to cooling has not yet created the central depression, and the fracture pattern is still entirely radial. Magellan MIDR quadrangle* containing this image: C1-45N011. Image resolution (m): 225. Size of region shown (E-W x N-S, in km): 439 x 474. Range of emissivities from violet to red: 0.82 -- 0.88. Vertical exaggeration: 100. Azimuth of viewpoint (deg clockwise from East): 150. Elevation of viewpoint (km): 600. *Quadrangle name indicates approximate center latitude (N=north, S=south) and center longitude (East).
Image Credit:
NASA/JPL/USGS


Latest Images Search Methods Animations Spacecraft & Telescopes Related Links Privacy/Copyright Image Use Policy Feedback Frequently Asked Questions Photojournal Home Page First Gov Freedom of Information Act NASA Home Page Webmaster
Bottom navigation bar