Cross-hatched Venus puzzles astronomers.Cross-hatched Venus puzzles astronomers Famous astronomers and astrophysicists include: Directory: A B C D E F G H I J K L M N O P Q R S T U V W X Y Z A
Magellan's radar views of cloud-enveloped Venus reveal some clearly unexpected new surface features. The most unusual one recorded since the craft began mapping the planet on Sept. 15 consists of a remarkably regular, cross-hatched pattern (left photo), formed when several parallel, linear features intersect a group of brighter ones at almost right angles. Researchers have never seen such terrain either on Venus or the other planets," says project scientist R. Stephen Saunders Multiple people share the name as Stephen Saunders:
Jet Propulsion Laboratory (JPL) is a NASA research center located in the cities of Pasadena and La Cañada Flintridge, near Los Angeles, California, USA. in Pasadona, Calif. The unusual pattern marks a low rise in the northern hemisphere between two plains called Sedna Planitia Sedna Planitia is a large lowland area of Venus. It is thought to be lava-covered and similar to a lunar mare. and Guinevere Planitia. Lines in the fainter of the two groups are regularly spaced about 1 kilometer apart, Saunders says, and are about as narrow as the radar can detect -- roughly 120 meters. The brighter of the cross-hatched lines are less regular, and in some places appear to begin where they intersect the faint lines. Magellan researchers do not know whether the lines represent fractures of some kind, but Saunders says that parts of the puzzling pattern look as though they may be associated with some past volcanic activity. Magellan has also returned images revealing two craters. Clear differences between them suggest the craters had vastly different origins. Features in the smaller, 1-km-diameter crater (upper right photo) indicate explosive volcanism volcanism or vulcanism Any of various processes and phenomena associated with the surface discharge of molten rock or hot water and steam, including volcanoes, geysers, and fumaroles. . For example, the radar-bright surface deposit that broadens away from the south side appears to have been created by erupted debris. About 37 km across, the larger crater (pictured at lower right), located in Guinevere Planitia, presents the classic look of a meteorite meteorite, meteor that survives the intense heat of atmospheric friction and reaches the earth's surface. Because of the destructive effects of this friction, only the very largest meteors become meteorites. impact. A lack of debris on the crater's south side suggests the meteorite was descending from the south at a shallow angle to the surface when it hit. The crater's central peak probably formed when the floor, compressed by the impact, rebounded. Other images include what Saunders describes as "lots" of low domes only a few kilometers across and resembling what some geophysicists say are shield volcanoes (SN: 6/23/90, p. 392). There is also "a very curious field of little craters, which have little sinuous sinuous /sin·u·ous/ (sin´u-us) bending in and out; winding. sinuous bending in and out; winding. channels coming out of them," Saunders says. |
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