mirrored file at http://SaturnianCosmology.Org/ For complete access to all the files of this collection see http://SaturnianCosmology.org/search.php ========================================================== [1][LINK] [2]Home [3]Table of Contents [4]What's New [5]Image Index [6]Copyright [7]Puzzles [8]Shopping [9]Search [10]Earth _Earth Introduction_ _My view of our planet was a glimpse of divinity. -Edgar Mitchell, USA_ Table of Contents Earth Introduction[11]Earth Statistics [12]Earth Movies [13]Views of the Earth Earth's Moon [14]The Moon Earth Science [15]Earth's Interior & Plate Tectonics[16]Earth From Space[17]Clouds From Space[18]Terrestrial Impact Craters[19]Terrestrial Impact Crater Structures[20]Chain of Impact Craters[21]Educator's Guide to Impact Craters[22]Terrestrial Volcanoes[23]Hawaiian Volcanoes[24]Valles Caldera, New Mexico[25]Shrinking of Greenland's Glaciers[26]IMAGE Spacecraft[27]Auroral Emmisions[28]Planetary Icosahedrons[29]Earth Image/Animation Gallery Internet Resources [30]Earth From Space[31]Earth Viewer [32][LINK] From the perspective we get on Earth, our planet appears to be big and sturdy with an endless ocean of air. From space, astronauts often get the impression that the Earth is small with a thin, fragile layer of atmosphere. For a space traveler, the distinguishing Earth features are the blue waters, brown and green land masses and white clouds set against a black background. Many dream of traveling in space and viewing the wonders of the universe. In reality all of us are space travelers. Our spaceship is the planet Earth, traveling at the speed of 108,000 kilometers (67,000 miles) an hour. Earth is the 3rd planet from the Sun at a distance of about 150 million kilometers (93.2 million miles). It takes 365.256 days for the Earth to travel around the Sun and 23.9345 hours for the Earth rotate a complete revolution. It has a diameter of 12,756 kilometers (7,973 miles), only a few hundred kilometers larger than that of Venus. Our atmosphere is composed of 78 percent nitrogen, 21 percent oxygen and 1 percent other constituents. Earth is the only planet in the solar system known to harbor life. Our planet's rapid spin and molten nickel-iron core give rise to an extensive magnetic field, which, along with the atmosphere, shields us from nearly all of the harmful radiation coming from the Sun and other stars. Earth's atmosphere protects us from meteors, most of which burn up before they can strike the surface. From our journeys into space, we have learned much about our home planet. The first American satellite, Explorer 1, discovered an intense radiation zone, now called the Van Allen radiation belts. This layer is formed from rapidly moving charged particles that are trapped by the Earth's magnetic field in a doughnut-shaped region surrounding the equator. Other findings from satellites show that our planet's magnetic field is distorted into a tear-drop shape by the [33]solar wind. We also now know that our wispy upper atmosphere, once believed calm and uneventful, seethes with activity -- swelling by day and contracting by night. Affected by changes in solar activity, the upper atmosphere contributes to weather and climate on Earth. Besides affecting Earth's weather, solar activity gives rise to a dramatic visual phenomenon in our atmosphere. When charged particles from the solar wind become trapped in Earth's magnetic field, they collide with air molecules above our planet's magnetic poles. These air molecules then begin to glow and are known as the [34]auroras or the [35]northern and southern lights. 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 Nitrogen Oxygen Other 77% 21% 2% Animations of Earth * [36]Rotation Earth Movie. * [37]Earth Topography Animation. * [38]Aurora Video. * [39]Earth/Venus Rotation Movie. * [40]Galileo Earth Encounter. * [41]Earth: The Movie - Animation of Clouds & Flight. * [42]Earth: The Movie - Animation of Clouds. Views of Earth The following set of images show some of the wonders of our planet, _the Earth_. [43]Earth [44]South America This color image of the Earth was obtained by [45]Galileo at about 6:10 a.m. Pacific Standard Time on Dec. 11, 1990, when the spacecraft was about 1.3 million miles from the planet. Galileo was making the first of two Earth flybys on its way to Jupiter. South America is near the center of the picture, and the white, sunlit continent of Antarctica is below. Picturesque weather fronts are visible in the South Atlantic, lower right. _(Courtesy NASA/USGS)_ [46]Africa [47]Africa The crew of Apollo 17 took this photograph of Earth in December 1972 while the spacecraft was traveling between the Earth and the Moon. The orange-red deserts of Africa and Saudi Arabia stand in stark contrast to the deep blue of the oceans and the white of both clouds and snow-covered Antarctica. _(Courtesy NASA)_ [48]Earth and Moon [49]Mariner 10's View of the Earth & Moon The Earth and Moon were imaged by [50]Mariner 10 from 2.6 million kilometers while completing the first ever Earth-Moon encounter by a spacecraft capable of returning high resolution digital color image data. These images have been combined below to illustrate the relative sizes of the two bodies. From this particular viewpoint the Earth appears to be a water planet! _(Courtesy NASA/JPL/Northwestern University)_ [51]Earth and Moon [52]The Earth & Moon During its flight, the Galileo spacecraft returned images of the Earth and Moon. Separate images of the Earth and Moon were combined to generate this view. The Galileo spacecraft took the images in 1992 on its way to explore the Jupiter system in 1995-97. The image shows a partial view of the Earth centered on the Pacific Ocean about latitude 20 degrees south. The west coast of South America can be observed as well as the Caribbean; swirling white cloud patterns indicate storms in the southeast Pacific. The distinct bright ray crater at the bottom of the Moon is the Tycho impact basin. The lunar dark areas are lava rock filled impact basins. This picture contains same scale and relative color/albedo images of the Earth and Moon. _(Courtesy USGS/NASA)_ [53]Northeast Africa and the Arabian Peninsula [54]Northeast Africa and the Arabian Peninsula This image of northeast Africa and the Arabian Peninsula was taken from an altitude of about 500,000 kilometers (300,000 miles) by the Galileo spacecraft on December 9, 1992, as it left Earth en route to Jupiter. Visible are most of Egypt (left of center), including the Nile Valley; the Red Sea (slightly above center); Israel; Jordan, and the Arabian Peninsula. In the center, below the coastal cloud, is Khartoum, at the confluence of the Blue Nile and the White Nile. Somalia (lower right) is partly covered by clouds. _(Courtesy NASA/JPL)_ [55]Horn of Africa [56]Horn of Africa, Somalia The orange and tan colors of this high-oblique photograph of the Horn of Africa indicate an arid-to-semiarid landscape in the northern half of the east African country of Somalia. Except in the darker areas where thicker vegetation can be found, most of the vegetation in this part of Somalia is shrub brush and grasslands. The general climate of this region features hot temperatures and scarce, irregular rainfall. Two distinct drainage basins are characterized by lighter colors-the Nugaaleed Valley along the western side of the photograph and the other watershed trending toward the Hafun Peninsula, the tombolo along the east coast of Somalia. The southern extent of the Saudi Arabian Peninsula is visible north across the Gulf of Aden. _(Courtesy NASA)_ [57]Greenland [58]Southern Tip of Greenland The southern tip of Greenland is seen in this high-oblique, almost colorless, stark photograph of the worlds largest island. The blackness of space contrasts sharply with the whiteness of clouds, ice, and snow. The only true color is the blue of the Atlantic Ocean and the Labrador Sea. Cloud-free conditions existing along the southern coastal area emphasize the deeply indented fjords along the coast. A close look at the white areas reveals three different features-snow and ice on the land; cloud formations over the central region and the eastern and western sides of the island; and wispy-looking ice floes off the southeast and the southwest tip of the fjord-lined coast, which are moved by the East Greenland Current to the south-southwest, and larger ice packs developing north along the east coast. Greenland has the only surviving continental glacier in the Northern Hemisphere. This ice sheet covers seven-eighths of Greenlands surface and contains an estimated 11 percent of the worlds fresh water. _(Courtesy NASA)_ [59]Antarctica [60]Antarctica This image of Antarctica was taken by Galileo several hours after it flew close to the Earth on December 8, 1990. This is the first picture of the whole Antarctic continent taken nearly at once from space. Galileo was about 200,000 kilometers (125,000 miles) from Earth when the pictures were taken. The icy continent is surrounded by the dark blue of three oceans: the Pacific to the left, the Indian to the bottom, and a piece of the Atlantic to the upper right. Nearly the entire continent was sunlit at this time of year, just two weeks before southern summer solstice. The arc of dark spots extending from near the South Pole (close to the center) toward the lower left is the Transantarctic Mountain Range. To the left of the mountains is the vast Ross Ice Shelf and the shelf's sharp border with the dark waters of the Ross Sea. The thin blue line along the Earth's [61]limb marks our planet's atmosphere. _(Courtesy NASA/JPL)_ [62]Earth Limb [63]Clementine Mission This false-colored image was acquired during the Clementine mission. It shows airglow of the upper atmosphere as a thin blue line. The bright spot toward the bottom is an urban area. _(Courtesy Naval Research Laboratory)_ [64]Earth Map [65]Map projected image of Earth (AVHRR) This image is a Homolosine projection of the Earth prepared from Advanced Very High Resolution Radiometer (AVHRR) image data. _(Courtesy ESA/NASA/NOAA/USGS/CSIRO)_ [66]Earth at Night [67]Earth Lights This view of earth shows the global city lights as seen by the Defense Meteorological Satellite. Eastern U.S., Europe, and Japan are brightly lit by their cities, while the interiors of Africa, Asia, Australia, and South America remain (for now) dark and lightly populated. _(Courtesy NASA/GSFC)_ [68]USA [69]USA This image is a mosaic of the United States prepared by using 16 images from the Advanced Very High Resolution Radiometer (AVHRR) sensors on the meteorological satellites NOAA-8 and NOAA-9. The images were acquired between May 24, 1984 and May 14, 1986. On false-color infrared mosaics, vegetation appears in various tones of red instead of green. The "redness" indicates vegetation density, type and whether growing on dry land or in a swamp (a mixture of reddish vegetation and dark blue surface water produces dark tones). Grasslands appear light red, deciduous trees and croplands appear red, and coniferous forests appear dark red or maroon. Desert areas appear white and urban areas (pavement and buildings) appear bluish green. Lakes, rivers and oceans appear in various shades of blue, dark blue for deep water and light blue for shallow or turbid water. Exposed bedrock generally appears as a dark bluish-green or other dark tone. _(Courtesy USGS)_ [70]HOME [71]Return to Venus [72]Voyage to Mars _Copyright © 1997-2001 by [73]Calvin J. Hamilton. All rights reserved._ [74]Privacy Statement. 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