2010 EK139
Encyclopedia
is a trans-Neptunian object
orbiting the Sun
in the scattered disc
. It was discovered in 2010 by astronomers from the OGLE
team led by Andrzej Udalski
from Warsaw University. With an absolute magnitude
(H) of 3.8, it is very likely a dwarf planet
.
around 2038, and is currently 39.1 AU
from the Sun.
It has been observed 122 times over 5 oppositions and has an orbit quality of 2. There are precovery
images dating back to 2002. A ten million year integration of the orbit shows that this object may be in a 7:2 resonance
with Neptune
.
Assuming a generic trans-Neptunian albedo of 0.09, it is about 770 km in diameter. But since the true albedo is unknown and it has an absolute magnitude of 3.8, it could easily be from about 462 to 1033 km in diameter.
Trans-Neptunian object
A trans-Neptunian object is any minor planet in the Solar System that orbits the Sun at a greater distance on average than Neptune.The first trans-Neptunian object to be discovered was Pluto in 1930...
orbiting the Sun
Sun
The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields...
in the scattered disc
Scattered disc
The scattered disc is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater...
. It was discovered in 2010 by astronomers from the OGLE
Ogle
Ogle may refer to:*ogle, to stareas, or from, a surname* The Ogle family of Northumberland, England** Benjamin Ogle, Governor of Maryland from 1798 to 1801** Sir Chaloner Ogle, 1st Baronet , British Admiral...
team led by Andrzej Udalski
Andrzej Udalski
Professor Andrzej Udalski, PhD is a Polish astronomer and director of the Astronomical Observatory of the University of Warsaw...
from Warsaw University. With an absolute magnitude
Absolute magnitude
Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth...
(H) of 3.8, it is very likely a dwarf planet
Dwarf planet
A dwarf planet, as defined by the International Astronomical Union , is a celestial body orbiting the Sun that is massive enough to be spherical as a result of its own gravity but has not cleared its neighboring region of planetesimals and is not a satellite...
.
Distance
It will come to perihelionApsis
An apsis , plural apsides , is the point of greatest or least distance of a body from one of the foci of its elliptical orbit. In modern celestial mechanics this focus is also the center of attraction, which is usually the center of mass of the system...
around 2038, and is currently 39.1 AU
Astronomical unit
An astronomical unit is a unit of length equal to about or approximately the mean Earth–Sun distance....
from the Sun.
It has been observed 122 times over 5 oppositions and has an orbit quality of 2. There are precovery
Precovery
Precovery is a term used in astronomy that describes the process of finding the image of an object in old archived images or photographic plates, for the purpose of calculating a more accurate orbit...
images dating back to 2002. A ten million year integration of the orbit shows that this object may be in a 7:2 resonance
Resonant trans-Neptunian object
In astronomy, a resonant trans-Neptunian object is a trans-Neptunian object in mean motion orbital resonance with Neptune. The orbital periods of the resonant objects are in a simple integer relations with the period of Neptune e.g. 1:2, 2:3 etc...
with Neptune
Neptune
Neptune is the eighth and farthest planet from the Sun in the Solar System. Named for the Roman god of the sea, it is the fourth-largest planet by diameter and the third largest by mass. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times...
.
Assuming a generic trans-Neptunian albedo of 0.09, it is about 770 km in diameter. But since the true albedo is unknown and it has an absolute magnitude of 3.8, it could easily be from about 462 to 1033 km in diameter.
External links
- OCKS: OGLE Carnegie Kuiper belt Survey (OCKS is a Southern sky survey searching for Kuiper-belt objects and dwarf planets)
- Orbital simulation from JPL (Java) / Horizons Ephemeris