Jack C. Davis Observatory Planetary Walkway Venus |
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Dedication: To Virgie - You are my Venus.
From your loving husband,
Bill Miller |
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| Named after the Roman goddess of love and beauty, Venus is very similar in size, mass, and composition to Earth. But the similarities end there, as Venus has no oceans, and its scorching temperatures of about 484°C could melt lead. |
Mean Distance from Sun 108.2 million kilometers |
Orbital Period 0.62 years |
Rotational Period 243 days (retrograde) |
Venus is the third brightest object in the sky just behind the Sun and the Moon. Venus is always covered with thick layers of clouds that reflect approximately 70 % of the light it receives from the Sun back out into space. Venus is often referred to as Earth's sister planet because it is our nearest planetary neighbor. It is just under ¾ the distance the Earth is from the Sun (0.73 A.U.) and maintains an average surface temperature of 730 K (815°F). Venus has the hottest natural temperatures of all the other planets in the Solar System even though Mercury is nearest to the Sun. Venus has an enormous runaway greenhouse effect produced by a 96.5% carbon dioxide atmosphere and along with other greenhouse gases efficiently traps heat near its surface.
Venus has no oceans or surface water, yet scientists think a few billion years ago it was Earth like, but something happened to its surface water. Venus has over 80% of the mass of the Earth and has two continent-sized features, called Ishtar Terra and Aphrodite Terra. Venus has a very slow rotation on its axis at 243 Earth days and rotates in the opposite direction as most of the planets. It is said to have retrograde rotation on its axis. A day on Venus is longer than the planets year of approximately 225 Earth days. Venus still has active volcanoes and its surface features change rapidly with extensive lava flows and high temperatures. The Soviet Venera 9 and 14 space mission took pictures at the surface under the clouds of Venus while America's NASA space satellite, Magellan took radar images through the clouds that revealed many of the surface features we now study. | | Previous: Mercury | Walkway Overview | Next: Earth |
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| The northern hemisphere is displayed in this global view of the surface of Venus. The north pole is at the center of the image, with 0 degrees, 90 degrees, 180 degrees, 270 degrees east longitudes at the 6, 3, 12, and 9 o'clock positions, respectively, of an imaginary clock face. Magellan synthetic aperture radar mosaics from the three eight-month cycles of Magellan radar mapping are mapped onto a computer-simulated globe to create this image. Magellan obtained coverage of 98 percent of the surface of Venus. Remaining gaps are filled with data from previous missions, (the Soviet Venera 15 and 16 radar and Pioneer Venus Orbiter altimetry) and data from Earth-based radar observations from the Arecibo radio telescope. Simulated color is used to enhance small-scale structures. The simulated hues are based on color images recorded by the Venera 13 and 14 landing craft. Maxwell Montes, the planet's highest mountain at 11 kilometers (6.6 miles) above the average elevation, is the bright feature in the lower center of the image. Other terrain types visible in this image include tessera, ridge belts, lava flows, impact craters and coronae. Image courtesy NASA Jet Propulsion Laboratory (NASA-JPL). |
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