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Astronomy Picture of the Day 4-27-03
NASA ^ | 4-27-03 | Robert Nemiroff and Jerry Bonnell

Posted on 04/26/2003 9:46:15 PM PDT by petuniasevan

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2003 April 27
See Explanation.  Clicking on the picture will download
 the highest resolution version available.

Venus' Once Molten Surface
Credit: E. De Jong et al. (JPL), MIPL, Magellan Team, NASA

Explanation: If you could look at Venus with radar eyes - this is what you might see. This computer reconstruction of the surface of Venus was created from data from the Magellan spacecraft. Magellan orbited Venus and used radar to map our neighboring planet's surface between 1990 and 1994. Magellan found many interesting surface features, including the large circular domes, typically 25-kilometers across, that are depicted above. Volcanism is thought to have created the domes, although the precise mechanism remains unknown. Venus' surface is so hot and hostile that no surface probe has lasted more than a few minutes.


TOPICS: Astronomy; Astronomy Picture of the Day; Science
KEYWORDS: dome; radar; venus

Vacation Announcement

I will be on vacation from June 2nd through June 9th.
If anyone would like to volunteer to post APOD during that time, please FReepmail me.
Otherwise the APOD will not be posted as I will be visiting relatives in California.

Venus has a few similarities to Earth. It's nearly the same size, is a rocky planet, and has an atmosphere. There the similarities end.

Compare the tables below.

Venus Statistics
Mass (kg) 4.869e+24
Mass (Earth = 1) .81476
Equatorial radius (km) 6,051.8
Equatorial radius (Earth = 1) .94886
Mean density (gm/cm^3) 5.25
Mean distance from the Sun (km) 108,200,000
Mean distance from the Sun (Earth = 1) 0.7233
Rotational period (days) -243.0187
Orbital period (days) 224.701
Mean orbital velocity (km/sec) 35.02
Orbital eccentricity 0.0068
Tilt of axis (degrees) 177.36
Orbital inclination (degrees) 3.394
Equatorial surface gravity (m/sec^2) 8.87
Equatorial escape velocity (km/sec) 10.36
Visual geometric albedo 0.65
Magnitude (Vo) -4.4
Mean surface temperature 482°C
Atmospheric pressure (bars) 92
Atmospheric composition
Carbon dioxide
Nitrogen
    Trace amounts of: Sulfur dioxide, water vapor,
    carbon monoxide, argon, helium, neon,
    hydrogen chloride, and hydrogen fluoride.


96% 
3+% 

Earth Statistics
Mass (kg) 5.976e+24
Mass (Earth = 1) 1.0000e+00
Equatorial radius (km) 6,378.14
Equatorial radius (Earth = 1) 1.0000e+00
Mean density (gm/cm^3) 5.515
Mean distance from the Sun (km) 149,600,000
Mean distance from the Sun (Earth = 1) 1.0000
Rotational period (days) 0.99727
Rotational period (hours) 23.9345
Orbital period (days) 365.256
Mean orbital velocity (km/sec) 29.79
Orbital eccentricity 0.0167
Tilt of axis (degrees) 23.45
Orbital inclination (degrees) 0.000
Equatorial escape velocity (km/sec) 11.18
Equatorial surface gravity (m/sec^2) 9.78
Visual geometric albedo 0.37
Mean surface temperature 15°C
Atmospheric pressure (bars) 1.013
Atmospheric composition
Nitrogen
Oxygen
Other

77%
21%
2%

This picture shows two different perspectives of Venus. On the left is a mosaic of images acquired by the Mariner 10 spacecraft on February 5, 1974. The image shows the thick cloud coverage that prevents optical observation of the planet's surface. The surface of Venus remained hidden until 1978 when the Pioneer Venus 1 spacecraft arrived and went into orbit about the planet on December 4th. The spacecraft used radar to map planet's surface, revealing a new Venus. Later in August of 1990 the Magellan spacecraft arrived at Venus and began its extensive planetary mapping mission. This mission produced radar images up to 300 meters per pixel in resolution. The right image show a rendering of Venus from the Pioneer Venus and Magellan radar images.

The above image comes from the Solarviews Venus image and movie gallery. Here's the URL for page one of seven:

http://www.solarviews.com/cap/index/venus1.html

1 posted on 04/26/2003 9:46:15 PM PDT by petuniasevan
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To: MozartLover; Joan912; NovemberCharlie; snowfox; Dawgsquat; viligantcitizen; theDentist; ...

2 posted on 04/26/2003 9:47:11 PM PDT by petuniasevan (I'm a lefty. Left-handed. The only kind of lefty I've ever been.)
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To: petuniasevan
Some say that Venus is tectonically inert, compared to Mars. Venus has very little deep energy input anymore. Tidal forces from the sun would be strong if Venus rotated more quickly, but all Venus has is an interaction with its atmosphere and a good amount of surface heating. At depth it is quiet.

All the same, Venus is an excellent candidate for terraforming some day. It would need to be moved to an orbit farther from the sun, and it should have a good-sized moon of its own. How to do that and drive real estate agents to a marketing frenzy?

3 posted on 04/26/2003 9:56:34 PM PDT by RightWhale (Theorems link concepts; proofs establish links)
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To: petuniasevan
Thanks for posting this one. I was at JPL in the flight control room, flying the Magellan.

An interesting note; if you look at a picture of the spacecraft, you will notice it is almost all white. You are looking at a multilayer insulation (MLI) of metalized Mylar, Dacron net, and Kapton with an outer layer of white woven quartz. The quartz is the white you see in the pics.

4 posted on 04/26/2003 10:33:12 PM PDT by RadioAstronomer
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To: petuniasevan
Thanks for the ping
5 posted on 04/27/2003 5:44:30 AM PDT by firewalk
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To: petuniasevan
Mmmmm........looks like melted cheese.;^)
6 posted on 04/27/2003 8:35:29 AM PDT by MozartLover
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To: petuniasevan
Great images.
Thanks for the ping.
7 posted on 04/27/2003 8:43:18 AM PDT by sistergoldenhair (Don't be a sheep. People hate sheep. They eat sheep.)
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To: petuniasevan
Great pics, petuniasevan!

Whenever I hear talk of Venus' hostile surface, I'm always reminded of the episodes of the $6 Million Man where Steve does battle with the Soviet probe that was supposed to land on Venus, but wound up wreaking havoc on Earth, instead.

You see, the lander was equipped to deal with the extreme temperatures and pressures, as mentioned above, and could move independently, so it was basically a tank that used its sampling arms to tear up anything that approached. And shooting it was supposed to be "impossible."
8 posted on 04/27/2003 6:37:54 PM PDT by BradyLS
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