tll me about pluto ,pratyusha

Pluto is smaller than 7 of the moons in the Solar System. It is about two-thirds smaller than Earth's moon. Because it is so small, many scientists don't consider it a planet at all. In 1999, a group of scientists attempted to re-classify Pluto as a comet. On August 24, 2006, Pluto's status was officially changed from planet to dwarf planet. For decades, children have been taught in school that there are nine planets in our Solar System. However, with this change, there are now only eight planets. Also because of this change, there is a new category of small planets known as plutoids.

The only spacecraft to get somewhat close to Pluto was the Hubble Space Telescope. Hubble was able to take pictures of Pluto and its moons for scientists to study. Little is known about Pluto and its moons because it is so far away.

Pluto

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In Roman mythology, Pluto (Greek: Hades) is the god of the underworld. The planet received this name (after many other suggestions) perhaps because it's so far from the Sun that it is in perpetual darkness and perhaps because "PL" are the initials of Percival Lowell.

Pluto was discovered in 1930 by a fortunate accident. Calculations which later turned out to be in error had predicted a planet beyond Neptune, based on the motions of Uranus and Neptune. Not knowing of the error, Clyde W. Tombaugh at Lowell Observatory in Arizona did a very careful sky survey which turned up Pluto anyway.

After the discovery of Pluto, it was quickly determined that Pluto was too small to account for the discrepancies in the orbits of the other planets. The search for Planet X continued but nothing was found. Nor is it likely that it ever will be: the discrepancies vanish if the mass of Neptune determined from the Voyager 2 encounter with Neptune is used. There is no Planet X. But that doesn't mean there aren't other objects out there, only that there isn't a relatively large and close one like Planet X was assumed to be. In fact, we now know that there are a very large number of small objects in the Kuiper Belt beyond the orbit of Neptune, some roughly the same size as Pluto.


Read more about Pluto  l  Pluto facts, pictures and information. by nineplanets.org

 

Pluto has not yet been visited by a spacecraft. Even the Hubble Space Telescope can resolve only the largest features on its surface (left and above). A spacecraft called New Horizons was launched in January 2006. If all goes well it should reach Pluto in 2015.

Fortunately, Pluto has a satellite, Charon. By good fortune, Charon was discovered (in 1978) just before its orbital plane moved edge-on toward the inner solar system. It was therefore possible to observe many transits of Pluto over Charon and vice versa. By carefully calculating which portions of which body would be covered at what times, and watching brightness curves, astronomers were able to construct a rough map of light and dark areas on both bodies.

nix and hydraIn late 2005, a team using the Hubble Space Telescope discovered two additional tiny moons orbiting Pluto. Provisionally designated S/2005 P1 and S/2005 P2, they are now known as Nix and Hydra. They are estimated to be between 50 and 60 kilometers in diameter.

Pluto's radius is not well known. JPL's value of 1137 is given with an error of +/-8, almost one percen


Read more about Pluto  l  Pluto facts, pictures and information. by nineplanets.org

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plzz thumps up

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Pluto animiert.gif
Computer-generated map of Pluto fromHubble images, synthesized true color[a] and among the highest resolutions possible with current technology.
Discovery
Discovered byClyde W. Tombaugh
Discovery dateFebruary 18, 1930
Designations
MPC designation134340 Pluto
PronunciationListeni/ˈplt/,[b]
Named afterPluto
Minor planet
category
AdjectivePlutonian
Orbital characteristics
Epoch J2000
Aphelion
  • 7,311,000,000 km
  • 48.871 AU
Perihelion
  • 4,437,000,000 km
  • 29.657 AU
(1989 Sep 05)[1]
Semi-major axis
  • 5,874,000,000 km
  • 39.264 AU
Eccentricity0.248 807 66
Orbital period
Synodic period366.73 days
Average orbital speed4.666 km/s
Mean anomaly14.86012204°[3]
Inclination
  • 17.141 75°
  • 11.88° to Sun's equator
Longitude of ascending node110.303 47°
Argument of perihelion113.763 29°
Satellites4
Physical characteristics
Mean radius
Surface area
  • 1.665×107 km2[c]
  • 0.033 Earths
Volume
  • 6.39×109 km3[d]
  • 0.0059  Earths
Mass
Mean density2.03 ± 0.06 g/cm3[4]
Equatorial surface gravity
Escape velocity1.229  km/s[f]
Sidereal rotation
period
Equatorial rotation velocity47.18 km/h
Axial tilt119.591 ± 0.014° (to orbit)[4][g]
North poleright ascension312.993°[6]
North poledeclination6.163°[6]
Albedo0.49–0.66 (geometric, varies by 35%)[7][8]
Surface temp.
 Kelvin
minmeanmax
33 K44 K55 K
Apparent magnitude13.65[8] to 16.3[9]
(mean is 15.1)[8]
Absolute magnitude (H)−0.7[10]
Angular diameter0.065" to 0.115"[8][h]
Atmosphere
Surfacepressure0.30 Pa (summer maximum)
Compositionnitrogenmethane,carbon monoxide[11]


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