Technology tips

Thursday, 24 August 2017

PLUTO (the dwaf planet)



Pluto was discovered by Clyde Tombaugh in 1930 and was originally considered to be theninth planet from the Sun. After 1992, its status as a planet was questioned following the discovery of several objects of similar size in the Kuiper belt. In 2005, Eris, a dwarf planet in the scattered disc which is 27% more massive than Pluto, was discovered. This led the International Astronomical Union(IAU) to define the term "planet" formally in 2006, during their 26th General Assembly. That definition excluded Pluto and reclassified it as a dwarf planet.
Pluto is the largest and second-most-massive known dwarf planet in the Solar System and the ninth-largest and tenth-most-massive known object directly orbiting the Sun. It is the largest known trans-Neptunian object by volume but is less massive than Eris. Like other Kuiper belt objects, Pluto is primarily made of ice and rock and is relatively small—about one-sixth the mass of the Moon and one-third its volume. It has a moderatelyeccentric and inclined orbit during which it ranges from 30 to 49 astronomical units or AU (4.4–7.4 billion km) from the Sun. This means that Pluto periodically comes closer to the Sun than Neptune, but a stable orbital resonance with Neptune prevents them from colliding. Light from the Sun takes about 5.5 hours to reach Pluto at its average distance (39.5 AU)

ESTIMATED SIZE FOR PLUTO
YearRadiusNotes
19931195 kmMillis, et AL (if no haze)
19931180 kmMillis, et al. (surface & haze)
19941164 kmYoung & Binzel
20061153 kmBuie, et al.
20071161 kmYoung, Young, & Buie
20111180 kmZalucha, et al.
20141184 kmLellouch, et al
20151187 kmNew Horizonsmeasurement (from optical data)
20171189.9 kmNew Horizonsmeasurement (from radio occultation data)

No comments:

Post a Comment