By Jen Schoeller
This identify introduces readers to strange sea creatures.
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This name introduces readers to strange sea creatures.
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Extra info for Biggest, Baddest Book of Sea Creatures
Dec. 7, 1631 June 6, 1761 Dec. 9, 1874 June 8, 2004 Dec. 11, 2117 June 11, 2247 Dec. 13, 2360 © 2007 Encyclopædia Britannica, Inc. Dec. 4, 1639 June 3, 1769 Dec. 6, 1882 June 6, 2012 Dec. 8, 2125 June 9, 2255 Dec. 10, 2368 Studying the transits of 1761 and 1769 helped astronomers determine a more accurate value for the distance between Earth and the sun. ) When viewed through an optical (visible-light) telescope, Venus appears yellow-white and fairly featureless because of its permanent veil of clouds.
The images were taken in ultraviolet light by the Transition Region and Coronal Explorer (TRACE) satellite in Earth orbit. The time between successive images was about seven minutes. Orbit and spin. Like all the planets, Mercury travels around the sun in an elliptical (oval-shaped) orbit. Mercury’s orbit is the most eccentric, or elongated, of all the planets. Its orbit is also the most tilted. The plane of Mercury’s orbit is tipped about 7 degrees relative to the ecliptic, or the plane of Earth’s orbit.
It extends from the surface up to about 6–9 miles (10–15 kilometers), depending on the latitude and season. In this layer, temperatures drop rapidly with altitude. Nearly all the planet’s water vapor, and thus most clouds, exists in the troposphere. It is also where most weather occurs. Temperature differences make the air in the troposphere relatively unstable. Sunlight heats air near the surface, and the lighter, warmer air tends to rise. Colder air, which is denser, tends to sink. This process is called convection.
Biggest, Baddest Book of Sea Creatures by Jen Schoeller