Matthew Berkowitz Science PLUTO 11-9-99 Pluto is the farthest planet from the Sun (usually) and by far the smallest. Pluto is smaller than seven of the solar systems moons (the Moon, Io, Europa, Ganymede, Callisto, Titan and Triton).
Orbit: 5, 913, 520, 000 km (39. 5 AU) from the Sun (average) Diameter: 2274 km Mass: 1. 27 e 22 kg 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 tenth planet. Pluto is the only planet that has not been visited by a spacecraft. Even the Hubble Space Telescope can resolve only the largest features on its surface Fortunately, Pluto has a satellite, Charon.
The Essay on Pluto Planet Orbit Astronomers
... of the planet Neptune. This was often believed due to similarities between Pluto and the Neptune moon Triton. Triton and Pluto have similar ... to make one orbit around the sun in comparison to Neptune. Pluto crossed in front of Neptune most recently in January of 1979 ... Kuiper Belt, and many small objects with properties similar to Pluto, questions arose about whether or not Pluto was just another one ...
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 bot bodies. Pluto’s radius is not well known. JPL’s value of 1137 is given with an error of +/-8, almost one percent.
Though the sum of the masses of Pluto and Charon is known pretty well (it can be determined from careful measurements of the period and radius of Charon’s orbit and Kepler’s Third Law), the individual masses of Pluto and Charon are difficult to determine because that requires determining their mutual motions around the center of mass of the system which requires much finer measurements – they ” re so small and far away that even HST has difficulty. The ratio of their masses is probably somewhere between 0. 084 and 0. 157; more observations are underway but we won’t get really accurate data until a spacecraft is sent. Pluto is the second most contrasty body in the Solar System (after Iapetus).
Exploring the origin of that contrast is one of the high-priority goals for the proposed Pluto Express mission.
There are some who think Pluto would be better classified as a large asteroid or comet rather than as a planet. Some consider it to be the largest of the Kuiper Belt objects (also known as Trans-Neptunian Objects).
There is considerable merit to the later position, but historically Pluto has been classified as a planet and it is likely to remain so. Pluto’s orbit is highly eccentric. At times it is closer to the Sun than Neptune (as it was from January 1979 thru February 11 1999).
Pluto rotates in the opposite direction from most of the other planets.
Pluto is locked in a 3: 2 resonance with Neptune; i. e. Pluto’s orbital period is exactly 1. 5 times longer than Neptune’s.
Its orbital inclination is also much higher than the other planets’. Thus though it appears that Pluto’s orbit crosses Neptune’s, it really doesn’t and they will never collide. Uranus, the plane of Pluto’s equator is at almost right angles to the plane of its orbit. The surface temperature on Pluto is not well known but is probably between 35 and 45 Kelvins (-228 to -238 C).
The Term Paper on Pluto Hubble Space Telescope
... before its atmosphere freezes. The atmospheric pressure deduced for Pluto's surface is 1/100, 000 that of Earth's surface pressure. Pluto was ... above or below the plane of Neptune's orbit. Under these conditions, Pluto and Neptune will not collide and do not ... (Courtesy NASA/ESA/ESO) Pluto, Charon, and USA Comparison This image shows the approximate size of Pluto and Charon by overlaying them ...
Pluto’s composition is unknown, but its density (about 2 gm / cm 3) indicates that it is probably a mixture of 70% rock and 30% water ice much like Triton. The bright areas of the surface seem to be covered with ices of nitrogen with smaller amounts of (solid) methane, ethane and carbon monoxide.
The composition of the darker areas of Pluto’s surface is unknown but may be due to primordial organic material or photochemical reactions driven by cosmic rays. Little is known about Pluto’s atmosphere, but it probably consists primarily of nitrogen with some carbon monoxide and methane. It is extremely tenuous the surface pressure being only a few micro bars. Pluto’s atmosphere may exist as a gas only when Pluto is near its perihelion; for the majority of Pluto’s long year, the atmospheric gases are frozen into ice. Near perihelion, it is likely that some of the atmosphere escapes to space perhaps even interacting with Charon. The Pluto Express mission planners want to arrive at Pluto while the atmosphere is unfrozen..
