Sep
21
2008
0

Solar System’s Fifth Dwarf Planet Named

On September 17, the International Astronomical Union announced that 2003 EL61 would be classified as the fifth named dwarf planet and officially designated Haumea. The name was chosen after meetings of the IAU’s Committee on Small Body Nomenclature and the Working Group for Planetary System Nomenclature. The number of dwarf planets is now five: Ceres, Eris, Haumea, Makemake and Pluto.

The 2,200 km ellipsoidal body—deformed due to a four-hour rotation period—is just beyond the orbit of Pluto and has two satellites. Orbiting among the Trans-Neptunian objects, Haumea is currently 50 astronomical units from the Sun but can get as close as 35 A.U. The astronomical unit is the average Earth-Sun distance and a standard measure of distance within the solar system.

In Hawaiian mythology, Haumea is the goddess of childbirth and fertility.

Written by Brent in: Space Exploration | Tags: , , , ,
Jun
14
2008
0

It’s Official: They’re Plutoids

Plutoids Pluto and Erix

Two years ago the International Astronomical Union (IAU) angered a lot of people when the Solar System’s ninth planet Pluto was demoted and designated a “dwarf planet” along with the asteroid Ceres and the recently discovered trans-neptunian object Eris. Well, the IAU has now come up with an official designation for Pluto and Eris that is almost guaranteed to upset people all over again. While some may think it’s a silly exercise to spend so much energy coming up with classification schemes (years ago the physicist Enrico Fermi complained about the number of sub-atomic particles saying “If I could remember the names of all these particles, I’d be a botanist.”), it is important for scientists to make classifications of the objects they study. The Greeks used the term “planetes astrum” to describe the wandering stars—as opposed to the “fixed” stars—but that definition did not really distinguish the actual planets from the Moon and Sun. But “Plutoid?”

The IAU Committee on Small Body Nomenclature defines a plutoid as “celestial bodies in orbit around the Sun at a semimajor axis greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighbourhood around their orbit.” For naming purposes, any body that meets these criteria and have an absolute magnitude brighter than H = +1 where H is the magnitude of the planet, asteroid, comet, etc. at one Astronomical Unit from the Sun.

In the above image, Pluto and its three moons are shown on the left while Eris is on the right.

Image Credit: IAU, NASA/ESA Hubble Space Telescope, H. Weaver (JHU/APL), A. Stern (SwRI), the HST Pluto Companion Search Team and M. Brown.

Written by Brent in: General Science | Tags: , , ,

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