Title: 2010 BK118
Content:   (also written 2010 BK118) is a centaur roughly 20–60 km in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of ~400 AU. came to perihelion in April 2012 at a distance of 6.1 AU from the Sun (outside the orbit of Jupiter). It has a Jupiter-MOID of 1.1 AU. , it is 11 AU from the Sun. It will not be 50 AU from the Sun until 2043. After leaving the planetary region of the Solar System, will have a barycentric aphelion of 791 AU with an orbital period of 8000 years.
Title: 2010 VR11
Content:  , also written 2010 VR11, is a Kuiper belt object with an absolute magnitude of 5.6. Assuming an albedo of 0.08, it is estimated to be about 350 km in diameter. Astronomer Mike Brown lists it as possibly a dwarf planet.
Title: 11 Orionis
Content:  11 Orionis is a solitary Ap star in the equatorial constellation of Orion, near the border with Taurus. It is visible to the naked eye with an apparent visual magnitude of 4.65, and it is located approximately 365 light years away from the Sun based on parallax. The star is moving further from the Sun with a heliocentric radial velocity of +16.8 km/s. This object is a chemically peculiar star, known as an Ap star, with enhanced silicon and chromium lines in its spectrum. It is an α² CVn variable, ranging from 4.65 to 4.69 magnitude with a period of 4.64 days. The magnetic field measured from metal lines has a strength of 160 G.
Title: (111253) 2001 XU10
Content:  orbits the Sun at a distance of 0.98–2.52 AU once every 2 years and 4 months (848 days; semi-major axis of 1.75 AU). Its orbit has an eccentricity of 0.44 and an inclination of 42° with respect to the ecliptic. The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in February 2000. is a member of the Apollo asteroids, the largest subgroup of near-Earth asteroids which cross the orbit of Earth. It is also a Mars-crosser, as it crosses the orbit of the Red Planet at 1.66 AU.
Title: 110 Herculis
Content:  110 Herculis (abbreviated to 110 Her) is a star in the northern constellation of Hercules. Its apparent magnitude is 4.19, and it can be faintly seen with the naked eye, according to the Bortle scale. Based on parallax estimates made by the Hipparcos spacecraft, the star is located fairly close, about 62.7 light-years (19.21 parsecs) away. 110 Herculis has a spectrum matching that of an F-type main-sequence star. It is about 1.4 to 1.7 times more massive than the Sun, and about two times wider than the Sun. Its effective temperature is about 6400 K. An infrared excess has been detected, indicating the presence of a circumstellar disk. 110 Herculis is the 17th-brightest star in the constellation. It is located in the sky about halfway between Rasalague in Ophiuchus and Albireo in Cygnus, offset a trifle west. 110 Herculis, along with its apparent neighbors 111 Herculis, 112 Herculis, and 113 Herculis lie close to the eastern edge of the constellation of Hercules.
Title: Gemini 11
Content: Mass: 8374 lb Perigee: 156.4 nmi ; Apogee: 739.2 nmi ; Inclination: 28.85° ; Period: 101.52 min  Highest orbit (followed twice):
Title: 11 Cephei
Content:  11 Cephei is a single star in the northern constellation of Cepheus, located 184 light years away from the Sun. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.55. The star has a relatively high proper motion, traversing the celestial sphere at the rate of 0.153 arc seconds per annum. It is moving closer to the Earth with a heliocentric radial velocity of −38 km/s. This is an aging giant star with a stellar classification of K0.5 III, having exhausted the hydrogen at its core and expanded. It is a red clump giant, which means it is currently on the horizontal branch and is generating energy through helium fusion at the core. 11 Cephei is 670 million years old with 2.4 times the mass of the Sun and 11 times the Sun's radius. It is radiating around 95 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 5,446 K.
Title: 11 Aquilae
Content:  11 Aquilae (abbreviated 11 Aql) is a single star in the equatorial constellation of Aquila. 11 Aquilae is the Flamsteed designation. It has an apparent visual magnitude of 5.2, which means it is faintly visible to the naked eye. Based upon an annual parallax shift of 20.9 mas, the distance to this star is approximately 156 ly. The brightness of this star is diminished by 0.33 in magnitude because of extinction from interstellar gas and dust. This is an F-type main sequence star with a stellar classification of F8 V. It is radiating about 15.4 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 6,118 K, giving it the yellow-white glow of an F-type star. 11 Aquilae has been listed as a candidate for membership in the Ursa Major Moving Group, but most likely does not belong to that association.
Title: 11P/Tempel–Swift–LINEAR
Content:  11P/Tempel–Swift–LINEAR is a periodic Jupiter-family comet in the Solar System. Ernst Wilhelm Leberecht Tempel (Marseille) originally discovered the comet on November 27, 1869, it was later observed by Lewis Swift (Warner Observatory) on October 11, 1880, and realised to be the same comet. After 1908 the comet became an unobservable lost comet, but on December 7, 2001, an object was found by the Lincoln Near-Earth Asteroid Research (LINEAR) program, and confirmed by previous images from September 10 and October 17 as being the same comet. The comet was not observed during the 2008 unfavorable apparition because the perihelion passage occurred when the comet was on the far side of the Sun. The comet was observed during the 2014 and 2020 apparitions.
Title: 110 Virginis
Content:  110 Virginis is a star in the zodiac constellation Virgo, located 195 light-years away from the Sun. It is visible to the naked eye as an orange-hued star with an apparent visual magnitude of 4.40. The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s. The stellar classification of 110 Virginis is K0.5 IIIb Fe–0.5, indicating that this is an evolved giant star with a mild underabundance of iron in its spectrum. At the age of 4.5 billion years old, it belongs to a sub-category of giants called the red clump, which means it is on the horizontal branch and is generating energy through the helium fusion at its core. Compared to the Sun, it has 167% of the mass but has expanded to 11 times the size. The enlarged photosphere has an effective temperature of 4,664 K and is radiating 76 times the Sun's luminosity.

Question: Verify the following claims with "True" or "False": The celestial body known as 1101 Clematis has a temperature of 155 kelvins and an apoapsis of 520906000.0 Kilometers.
Answer: True