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(237) Coelestina

(225) Henrietta

(225088) 2007 OR10 is a trans-Neptunian object (TNO) orbiting the Sun in the scattered disc, approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System past the orbit of Neptune, and the largest known body in the Solar System without a name. According to current estimates as of May 2016, it is slightly larger than Makemake or Haumea, and is hence almost certainly a dwarf planet. It has one known moon.

(230965) 2004 XA192 is a Kuiper-belt object with a diameter of 7005339000000000000♠339+120−95 km. It has an absolute magnitude of 4.11. It was discovered on 12 December 2004 at Palomar Observatory.It is currently at 35.8 AU from the Sun, near its perihelion.

yes

(22) Kalliope I Linus

(236) Honoria

and [[#Satellite

(222) Lucia

(219774) 2001 YY145 is a stony asteroid and exceptionally slow rotator from the middle region of the asteroid belt, approximately 1.5 kilometers in diameter. It was discovered on 18 December 2001, by the U.S. Lowell Observatory Near-Earth-Object Search (LONEOS) at Anderson Mesa Station near Flagstaff, Arizona.The S-type asteroid orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,514 days).

(230) Athamantis

(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.

(234) Barbara

(232) Russia

(229) Adelinda

left

(2106) Hugo

(229762) 2007 UK126, also written as (229762) 2007 UK126, is a scattered disc object (SDO) with a bright absolute magnitude of 3.7. This makes it probably a dwarf planet. As of August 2011, Mike Brown lists it as highly likely a dwarf planet. Its light-curve amplitude is estimated to be Δm = 0.03 ± 0.01 mag.Its orbital eccentricity of 0.49 suggests that it was gravitationally scattered onto its eccentric orbit.

(214869) 2007 PA8 is an Apollo near-Earth asteroid roughly 1.6 km in diameter that came within 6.5 million km (4 million miles, 17 lunar distances) of Earth on November 5, 2012. It was discovered on August 9, 2007 by LINEAR. It was studied by the 70 m (230 ft) Goldstone Deep Space Network antenna as it came near Earth, which resulted in radar images and other data about the asteroid, such as its rotation rate.

(231) Vindobona

(233) Asterope

(226) Weringia

Resonance. A preliminary motion analysis of librating in a 3:10 resonance with Neptune. The animated GIF consists of 16 frames covering 26,000 years. Neptune is held stationary.

(213) Lilaea

(235) Carolina

(220) Stephania

(221) Eos

(227) Philosophia

(2162) Anhui

(219) Thusnelda

main-belt

(224) Oceana

(214) Aschera

Spacewatch from Kitt Peak

(228) Agathe

(215) Oenone

>, presumably

(216) Kleopatra

(2177) Oliver

(212) Medea

(217) Eudora

(22543) Ranjan

(218) Bianca

(223) Rosa

(211) Isolda

(214869) 2007 PA8 is an Apollo near-Earth asteroid roughly 1.6 km in diameter that came within 6.5 million km (4 million miles, 17 lunar distances) of Earth on November 5, 2012. It was discovered on August 9, 2007 by LINEAR. It was studied by the 70 m (230 ft) Goldstone Deep Space Network antenna as it came near Earth, which resulted in radar images and other data about the asteroid, such as its rotation rate. It has an Apollo type orbit and is classified as a potentially hazardous asteroid (PHA).(214869) 2007 PA8 may be a dormant comet related to the November γ Pegasids meteor shower.

The orbit of compared to the orbit of Eris, Pluto, and the outer planets

(229762) 2007 UK126, also written as (229762) 2007 UK126, is a scattered disc object (SDO) with a bright absolute magnitude of 3.7. This makes it probably a dwarf planet. As of August 2011, Mike Brown lists it as highly likely a dwarf planet. Its light-curve amplitude is estimated to be Δm = 0.03 ± 0.01 mag.Its orbital eccentricity of 0.49 suggests that it was gravitationally scattered onto its eccentric orbit. It will come to perihelion in February 2046.It has been observed 73 times over 11 oppositions with precovery images back to 1982.

(219774) 2001 YY145 is a stony asteroid and exceptionally slow rotator from the middle region of the asteroid belt, approximately 1.5 kilometers in diameter. It was discovered on 18 December 2001, by the U.S. Lowell Observatory Near-Earth-Object Search (LONEOS) at Anderson Mesa Station near Flagstaff, Arizona.The S-type asteroid orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,514 days). Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic. The first precovery was taken at Lincoln Lab's ETS in October 2001, extending the asteroid's observation arc by 2 months prior to its discovery observation.A rotational light-curve was obtained for this asteroid from photometric observations at the Californian Palomar Transient Factory in October 2013. It gave a rotation period of 1007.7 hours with an estimated error margin of ±86 hours. According to the Light Curve Data Base, it is the 11th slowest rotating minor planet known to exist. Due to its high brightness variation of 0.86 magnitude, the body is likely to have a non-spheroidal shape (U=2).The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.54 kilometers, based on an absolute magnitude of 16.43.

(23) Thalia

(22) Kalliope