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: 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: Expedition 11
Content: Perigee: ~384 km ; Apogee: ~396 km ; Inclination: ~51.6° ; Orbital period: ~92 min 
Title: Tempel 1
Content:  Comets are in unstable orbits that evolve over time due to perturbations and outgassing. Tempel 1 passed within 0.04 AU – or 5.9 million km (3.7 million mi) – of the dwarf planet Ceres on November 11, 2011. Then, as a Jupiter-family comet, it will spend years interacting with the giant planet Jupiter, finally passing within 0.02 AU – or 3.0 million km (1.9 million mi) – of Mars on October 17, 2183.
Title: 11 Camelopardalis
Content:   11 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis, located around 710 light years away from the Sun as determined by parallax. It has the variable star designation BV Camelopardalis; 11 Camelopardalis is the Flamsteed designation. This object is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of +5.22. It forms a double star with 12 Camelopardalis, which is only 3 arcminutes away. This is a main sequence Be star with a stellar classification of B3 Ve. Samus et al. (2017) classify it as a Be variable, rather than a Gamma Cassiopeiae type, and it ranges in magnitude from a peak of 5.10 down to 5.22. The star is spinning with a projected rotational velocity of 95 km/s, but is being viewed from an extreme pole-on position. Hence it is spinning much more rapidly than indicated. Outbursts of hydrogen emission lines have been observed, as well as rapid changes in hydrogen line profiles. It is 25 million years old with around six times the mass of the Sun.
Title: 2011 EO40
Content:  was discovered by Richard A. Kowalski on 10 March 2011 while observing for the Mount Lemmon Survey. Its orbit is typical of Apollo asteroids and is characterized by significant eccentricity (0.54), low inclination (3.36º), and a semi-major axis of 1.65 AU. Upon discovery, it was classified as an Earth crosser, a near-Earth asteroid (NEA) and a potentially hazardous asteroid (PHA) by the Minor Planet Center. It was listed on the Sentry Risk Table for less than one day. Its orbit is in need of additional observations to determine if it is part of an asteroid family; as of October 2015 the orbit is determined using just twenty observations spanning an observation arc of 34 days. has an absolute magnitude of 21.5, which gives a characteristic diameter of about 200 m.
Title: 118P/Shoemaker–Levy
Content:  118P/Shoemaker–Levy (also known as periodic comet Shoemaker–Levy 4) is a comet discovered by astronomers Carolyn and Eugene M. Shoemaker and David Levy. During the 2010 apparition the comet became as bright as apparent magnitude 11.5. The comet nucleus is estimated to be 4.8 kilometers in diameter. On December 3, 2015, comet Shoemaker–Levy 4 will pass 0.0442 AU from asteroid 4 Vesta. This comet should not be confused with Comet Shoemaker–Levy 9 (D/1993 F2) which spectacularly crashed into Jupiter in 1994.
Title: 2010 EU65
Content:  Sun at a distance of 17.0–22.9 AU once every 89 years and 3 months (32,606 days; semi-major axis of 19.97 AU). Its orbit has an eccentricity of 0.15 and an inclination of 15° with respect to the ecliptic. It has a Tisserand's parameter with respect to Jupiter (TJ) of 2.94, near the threshold of 3, typically used to distinguish asteroids from Jupiter-family comets. On 21 June 2021, the object came to perihelion at 17.0 AU and has since been moving away from the Sun. the object is at 17.009 AU, with a apparent magnitude of 21.71. The body's observation arc begins with a precovery observation taken by the Mount Lemmon Survey in April 2009.
Title: C/2013 US10 (Catalina)
Content:  0.82 AU from the Sun. At perihelion, it had a velocity of 46.4 km/s with respect to the Sun which is slightly greater than the Sun's escape velocity at that distance. It crossed the celestial equator on 17 December 2015 becoming a northern hemisphere object. On 17 January 2016 the comet will pass 0.72 AU from Earth and should be around magnitude 6 while located in the constellation of Ursa Major. is dynamically new. It came from the Oort cloud with a loosely bound chaotic orbit that was easily perturbed by galactic tides and passing stars. Before entering the planetary region (epoch 1950), had an orbital period of several million years. After leaving the planetary region (epoch 2050), it will be on an ejection trajectory.
Title: 21 Comae Berenices
Content:  a period of just over two days. Samus et al. (2017) have it classified as a low-amplitude Delta Scuti variable, although this is disputed. The age of the Melotte 111 cluster, and therefore this star, lies in the range of 400–800 million years. The star has a projected rotational velocity of 63 km/s, with a polar inclination of 64° or greater, resulting in a rotation period of 2.05 days. Stellar evolutionary models yield a mass of around 2.3 times that of the Sun and 2.6 times the Sun's radius for this object. It is radiating 38 times the luminosity of the Sun from its photosphere at an effective temperature of 8,900 K.

Question: Verify the following claims with "True" or "False": With a temperature of 155 kelvins, 1101 Clematis, has an escape velocity of 0.02 kilometres per second, and an apoapsis of 520906000.0 kilometres.
Answer: True