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

PIA01544: Venus
Target Name: Venus
Is a satellite of: Sol (our sun)
Mission: Hubble Space Telescope
Spacecraft: Hubble Space Telescope
Instrument: Imaging Science Subsystem - Narrow Angle
Product Size: 170 samples x 248 lines
Produced By: JPL
Producer ID: PIA01544
Addition Date: 1999-05-18
Primary Data Set: Space Telescope Science Institute
Full-Res TIFF: PIA01544.tif (48.41 kB)
Full-Res JPEG: PIA01544.jpg (3.494 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:
VENUS CLOUD TOPS VIEWED BY HUBBLE. This is a NASA Hubble Space Telescope ultraviolet-light image of the planet Venus, taken on January 24 1995, when Venus was at a distance of 70.6 million miles (113.6 million kilometers) from Earth. Venus is covered with clouds made of sulfuric acid, rather than the water-vapor clouds found on Earth. These clouds permanently shroud Venus' volcanic surface, which has been radar mapped by spacecraft and from Earth-based telescope. At ultraviolet wavelengths cloud patterns become distinctive. In particular, a horizontal "Y"-shaped cloud feature is visible near the equator. Similar features were seen from Mariner 10, Pioneer Venus, and Galileo spacecrafts. This global feature might indicate atmospheric waves, analogous to high and low pressure cells on Earth. Bright clouds toward Venus' poles appear to follow latitude lines. The polar regions are bright, possibly showing a haze of small particles overlying the main clouds. The dark regions show the location of enhanced sulfur dioxide near the cloud tops. From previous missions, astronomers know that such features travel east to west along with the Venus' prevailing winds, to make a complete circuit around the planet in four days. Because Venus is closer to the Sun than Earth, the planet appears to go through phases, like the Moon. When Venus swings close to Earth the planet's disk appears to grow in size, but changes from a full disk to a crescent. The image was taken with the Wide Field Planetary Camera-2, in PC mode. False color has been used enhance cloud features.
Image Credit:
NASA/JPL


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