Neil A. Armstrong
Neil A. Armstrong, the first man to walk on the moon, was born in Wapakoneta, Ohio, on August 5, 1930. He began his NASA career in Ohio.
After serving as a naval aviator from 1949 to 1952, Armstrong joined the National Advisory Committee for Aeronautics (NACA) in 1955. His first assignment was with the NACA Lewis Research Center (now NASA Glenn) in Cleveland. Over the next 17 years, he was an engineer, test pilot, astronaut and administrator for NACA and its successor agency, the National Aeronautics and Space Administration (NASA).
As a research pilot at NASA's Flight Research Center, Edwards, Calif., he was a project pilot on many pioneering high speed aircraft, including the well known, 4000-mph X-15. He has flown over 200 different models of aircraft, including jets, rockets, helicopters and gliders.
Armstrong transferred to astronaut status in 1962. He was assigned as command pilot for the Gemini 8 mission. Gemini 8 was launched on March 16, 1966, and Armstrong performed the first successful docking of two vehicles in space.
As spacecraft commander for Apollo 11, the first manned lunar landing mission, Armstrong gained the distinction of being the first man to land a craft on the moon and first to step on its surface.
Armstrong subsequently held the position of Deputy Associate Administrator for Aeronautics, NASA Headquarters, Washington, D.C. In this position, he was responsible for the coordination and management of overall NASA research and technology work related to aeronautics.
He was Professor of Aerospace Engineering at the University of Cincinnati between 1971-1979. During the years 1982-1992, Armstrong was chairman of Computing Technologies for Aviation, Inc., Charlottesville, Va.
He received a Bachelor of Science Degree in Aeronautical Engineering from Purdue University and a Master of Science in Aerospace Engineering from the University of Southern California. He holds honorary doctorates from a number of universities.
Armstrong is a Fellow of the Society of Experimental Test Pilots and the Royal Aeronautical Society; Honorary Fellow of the American Institute of Aeronautics and Astronautics, and the International Astronautics Federation.
He is a member of the National Academy of Engineering and the Academy of the Kingdom of Morocco. He served as a member of the National Commission on Space (1985-1986), as Vice-Chairman of the Presidential Commission on the Space Shuttle Challenger Accident (1986), and as Chairman of the Presidential Advisory Committee for the Peace Corps (1971-1973).
Armstrong has been decorated by 17 countries. He is the recipient of many special honors, including the Presidential Medal of Freedom; the Congressional Space Medal of Honor; the Explorers Club Medal; the Robert H. Goddard Memorial Trophy; the NASA Distinguished Service Medal; the Harmon International Aviation Trophy; the Royal Geographic Society's Gold Medal; the Federation Aeronautique Internationale's Gold Space Medal; the American Astronautical Society Flight Achievement Award; the Robert J. Collier Trophy; the AIAA Astronautics Award; the Octave Chanute Award; and the John J. Montgomery Award.
Showing posts with label THE MOON. Show all posts
Showing posts with label THE MOON. Show all posts
Thursday, July 7, 2011
INSIDE THE MOON
INSIDE THE MOON
The interior of the moon is layered into a hard, outer crust, a rigid outer mantle, a semi-rigid inner mantle, and a core. The interior of the moon is cooler than the interior of the Earth. Since the moon is so small (and so its surface area to volume ratio is large compared to that of the Earth), it loses its heat quickly into space. Since the Earth and the moon formed, the moon has cooled down much more than the Earth.
Crust: The moon's surface is dry, dusty and rocky. The rocky crust is about 37 miles (60 km) thick on the side of the moon that faces Earth and about 62 miles (100 km) thick on the opposite side of the Moon. Radioactive dating of moon rocks from NASA's Apollo mission dates the formation of the moon from about 4.3 billion years ago (about 60 million years after the formation of the Earth). Moon rocks that have been analyzed by NASA are similar to Earth rocks, but are richer in the elements aluminum and titanium. When the minerals Armalcolite (named for the three astronauts on NASA's Apollo 11: Neil A. ARMstrong, Buzz ALdrin, and Michael COLlins), Tranquillityite, and Pyroxferroite were found on the moon, they were not known on the Earth. At least some of these minerals have since been found on the Earth.
Rigid lithospheric mantle: This rocky layer is not hot enough to flow. This hard shell is about 620 miles (1,000 km) thick.
Non-rigid mantle: Only the deepest parts of this asthenospheric layer (rock which is less rigid than in a lithosphere but rigid enough to transmit seismic waves) are hot enough to flow.
Core: The non-fluid core may be composed of iron-rich rock. The core contains only about 2-4 percent of the Moon's total mass; this core is probably about 225 miles (360 km) in diameter).
This small, non-fluid core does not create much of a magnetic field; the moon's magnetic field is about one ten-millionth of the Earth's magnetic field. A compass wouldn't work on the moon, but since the sky is always dark (because there is no atmosphere), you could navigate by looking at the stars.
Crust: The moon's surface is dry, dusty and rocky. The rocky crust is about 37 miles (60 km) thick on the side of the moon that faces Earth and about 62 miles (100 km) thick on the opposite side of the Moon. Radioactive dating of moon rocks from NASA's Apollo mission dates the formation of the moon from about 4.3 billion years ago (about 60 million years after the formation of the Earth). Moon rocks that have been analyzed by NASA are similar to Earth rocks, but are richer in the elements aluminum and titanium. When the minerals Armalcolite (named for the three astronauts on NASA's Apollo 11: Neil A. ARMstrong, Buzz ALdrin, and Michael COLlins), Tranquillityite, and Pyroxferroite were found on the moon, they were not known on the Earth. At least some of these minerals have since been found on the Earth.
Rigid lithospheric mantle: This rocky layer is not hot enough to flow. This hard shell is about 620 miles (1,000 km) thick.
Non-rigid mantle: Only the deepest parts of this asthenospheric layer (rock which is less rigid than in a lithosphere but rigid enough to transmit seismic waves) are hot enough to flow.
Core: The non-fluid core may be composed of iron-rich rock. The core contains only about 2-4 percent of the Moon's total mass; this core is probably about 225 miles (360 km) in diameter).
This small, non-fluid core does not create much of a magnetic field; the moon's magnetic field is about one ten-millionth of the Earth's magnetic field. A compass wouldn't work on the moon, but since the sky is always dark (because there is no atmosphere), you could navigate by looking at the stars.
THE MOON
THE MOON
THE MOON'S ORBIT
The moon revolves around the Earth in about one month (27 days 8 hours). It rotates around its own axis in the same amount of time. The same side of the moon always faces the Earth; it is in a synchronous rotation with the Earth.
SAROS
The saros is the roughly 18-year periodic cycle of the Earth-Moon-Sun system. Every 6,585 days, the Earth, Moon and Sun are in exactly the same position. When there is a lunar eclipse, there will also be one exactly 6,585 days later.
SIZE
The gravitational tidal influence of the Moon on the Earth is about twice as strong as the Sun's gravitational tidal influence. The Earth:moon size ratio is quite small in comparison to ratios of most other planet:moon systems (for most planets in our Solar System, the moons are much smaller in comparison to the planet and have less of an effect on the planet).
MASS AND GRAVITY
The moon's gravitational force is only 17% of the Earth's gravity. For example, a 100 pound (45 kg) person would weigh only 17 pounds (7.6 kg) on the Moon.
The moon's density is 3340 kg/m 3. This is about 3/5 the density of the Earth.
The temperature on the Moon ranges from daytime highs of about 130°C = 265°F to nighttime lows of about -110°C = -170°F
ATMOSPHERE
The moon has no atmosphere. On the moon, the sky is always appears dark, even on the bright side (because there is no atmosphere). Also, since sound waves travel through air, the moon is silent; there can be no sound transmission on the moon.
MARE
CRATERS AND RILLES
The lunar crater Aristarchus ( on the NW edge of the Oceanus Procellarum). This huge, circular crater is 25 miles (40 km) in diameter and 2.2 miles (3.6 km) deep (from rim to floor). There is a lot of ejecta (material thrown from the crater at impact) surrounding the crater. |
These craters range in size up to many hundreds of kilometers, but the most enormous craters have been flooded by lava, and only parts of the outline are visible. The low elevation maria (seas) have fewer craters than other areas. This is because these areas formed more recently, and have had less time to be hit. The biggest intact lunar crater is Clavius which is 100 miles (160 km) in diameter.
MOON OR DOUBLE PLANET?
The Earth and the Moon are relatively close in size (4:1 in diameter, 81:1 in mass), unlike most planet/moon systems. Many people consider the Earth and Moon to be a double planet system (rather than a planet/moon system). The moon does not actually revolve around the Earth; it revolves around the Sun in concert with the Earth (like a double planet system).
LIBRATION
Libration is a rocking movement of the Moon. Librations cause us to view the Moon from different angles at different times, enabling us to see about 59 percent of the Moon's surface from Earth, even though the same side always faces us. There are librations due to variations in the rate of the Moon's orbital motion (longitudinal libration) and to the inclination of the Moon's equator with respect to its orbital plane (latitudinal libration). There is also an apparent libration due to an observer on Earth viewing the Moon from different angles as the Earth rotates (diurnal libration, which occurs each day). TWO LUNAR MONTHS
The sidereal and synodic lunar months have different lengths. The sidereal month is the amount of time it takes the Moon to return to the same position in the sky with respect to the stars; the sidereal month is 27.321 days long. The synodic month is the time between similar lunar phases (e.g., between two full moons); the synodic month is 29.530 days long.
LUNAR EXPLORATION
Astronaut Buzz Aldrin's footprint on the moon's Sea of Tranquility, from the Apollo 11 mission in 1969. |
MOON ROCKS
THE ORIGIN OF THE MOON
Most scientists believe that the moon was formed from the ejected material after the Earth collided with a Mars-sized object. This ejected material coalesced into the moon that went into orbit around th Earth. This catastrophic collision occurred about 60 million years after Earth itself formed (about 4.3 billion years ago). This is determined by the radioisotope dating of moon rocks
BLUE MOON
When two full moons occur in a single month, the second full moon is called a "Blue Moon." Another definition of the blue moon is the third full moon that occurs in a season of the year which has four full moons (usually each season has only three full moons.)
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