-
All roads and facilities are open
The Visitor Center is open daily from 8 a.m. to 4:30 p.m. Obtain a permit before entering any authorized cave.
Beyond the Moon
Mars Mars may not have always been the dry, cold planet it is now. Because of a thin atmosphere, it has been constantly bombarded by meteors. Go back to Activity #1 and review volcanic features on the Earth and Moon if needed. Then, take a look at the images below to identify Martian volcanic features.
M1 Mars Image 1
M2 Mars Image 2
M3 Mars Image 3
M4 Mars Image 4
M5 Mars Image 5
M6 Mars Image 6
Venus Until the advent of radar imaging in the '60's, the surface of Venus had been hidden from view. The absence of water on Venus may explain why it has a dense atmosphere made up mostly of carbon dioxide. Radar is able to penetrate that thick layer. It reflects differently off smooth or rough areas producing a black and white image. Regions that are bright are considered to be rough and dark areas are considered to be smooth. Therefore when viewing images of Venus, one must realize that not all large lava flows will be black. It is important to look for other clues to volcanic features. Examine the images below to identify Venusian volcanic features.
V1 Venus Image 1 V2 Venus Image 2
V3 Venus Image 3
V4 Venus Image 4
V5 Venus Image 5
V6 Venus Image 6
V7 Venus Image 7
B1 Bonus Image 1
B2 Bonus Image 2
B3 Bonus Image 3
B4 Bonus Image 4
|
Did You Know?
Watch out for bombs! Before they cooled, volcanic bombs were hot globs of lava that were hurled from volcanoes along the Great Rift. They form a variety of interesting shapes described as "breadcrust", "spindle" and "ribbons" by geologists.