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
|
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
|
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:
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?
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.