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: Kepler-11c
Content:  Kepler-11c has a mass of 13.5 ME and a radius of 3.15 RE, making it over 13.5 times the mass of earth, but approximately 3.15 times its radius. Neptune, in comparison, has a radius approximately 3.9 times that of Earth. With a density of 2.3 grams/cm3, Kepler-11c has a mass over double of that of pure water at 0 °C; it is also denser than all the Sun's gas giants, but less dense than any of its rocky planets. Its density is closest to the dwarf planet Pluto. Due in part to its proximity to its star, the planet's equilibrium temperature is 833 K, about three times hotter than Earth's average temperature. It orbits Kepler-11 every 13.02502 days at a distance 
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: KELT-11b
Content:  KELT-11b is an exoplanet orbiting around the yellow subgiant star KELT-11 about 320 light-years away from Earth. It is an inflated planet, one of the "puffiest planets" known, as a result of its close orbiting distance with its parent star. It has a radius 1.37 times that of Jupiter, but only 19% of its mass. It was discovered in 2016. The transmission spectrum study in 2020 have revealed the KELT-11b atmosphere containing sub-solar amount of water vapor, but significant amounts of hydrogen cyanide, together with oxides of titanium and aluminum. Also, the nightside flux do indicate a generally cloud-free atmosphere with an effective heat redistribution between dayside and nightside. Later studies have indicated the hydrogen cyanide spectral features are not well distinguished from spectral lines of carbon dioxide and carbon monoxide, although carbon dioxide seems to be present in larger amounts, indicating a high carbon/oxygen ratio of the planet.
Title: Kepler-11c
Content:  Kepler-11c is an exoplanet discovered in the orbit of the Sun-like star Kepler-11 by the Kepler spacecraft, a NASA telescope aiming to discover Earth-like planets. It is the second planet from its star, and is most likely a water planet with a thin hydrogen–helium atmosphere. Kepler-11c orbits Kepler-11 every 10 days, and has an estimated density twice that of pure water. It is estimated to have a mass thirteen times that of Earth and a radius three times that of Earth. Kepler-11c and its five sister planets form the first discovered system with more than three transiting planets. The Kepler-11 system also holds the record of being the most compact and the flattest system discovered. Kepler-11c and the other Kepler-11 planets were announced to the public on February 2, 2011, and was published in Nature a day later.
Title: Kepler-11f
Content:  Kepler-11 is a G-type star, much like the Sun is, and is located 659 parsecs away in the Cygnus constellation. It has 95% the mass and 110% the radius of the Sun. Its mass and radius, combined with an approximate iron content (metallicity) of 0 and effective temperature of 5680 K, makes the star very similar to the Sun, though slightly more diffuse and slightly cooler. However, the star is approximately 1.74 times the age of the Sun, and is estimated to have existed for eight billion years. Kepler-11 has six known planets in orbit: Kepler-11b, Kepler-11c, Kepler-11d, Kepler-11e, Kepler-11f, and Kepler-11g. Kepler-11's five inner planets orbit closely to their host star, and their orbits would fit within that of Mercury's. With an apparent magnitude of 14.2, Kepler-11 cannot be seen with the naked eye.
Title: Kepler-11c
Content:  Kepler-11c's host star, Kepler-11, is a G-type star 2,000 light-years away in the Cygnus constellation. With a mass of .95 Msun, a radius of 1.1 Rsun, a metallicity of [Fe/H] = 0, and an effective temperature of 5680 (± 100) K, Kepler-11 is almost identical to the Sun in terms of radius, mass, and temperature. However, Kepler-11 is much older than the Sun, with an estimated age of 8 (± 2) billion years (the Sun is approximately 4.6 billion years old ). Along with Kepler-11c, Kepler-11 is host to the planets Kepler-11b, Kepler-11d, Kepler-11e, Kepler-11f, and Kepler-11g. The inner five planets' orbits would fit within the orbit of planet Mercury, while Kepler-11g orbits Kepler-11 at a much further distance in comparison to the inner components. With an apparent magnitude of 14.2, Kepler-11 cannot be seen from Earth with the naked eye.
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: HATS-11b
Content:  HATS-11b has been described to be similar to Jupiter and orbits a subsolar metallicity star which is about 2955 light years away (906 parsecs). HATS-11b has an orbital period of around 3.6 Earth days and its temperature has been calculated to be 1637 Kelvin (1363.85 Celsius). HATS-11b has a mass of 0.85 and a radius of 1.49. The planet's orbital eccentricity is <0.34 which is an elliptical orbit.
Title: Kepler-11
Content:  Kepler-11 is a G-type star that is approximately 104% the mass of and 102% the radius of the Sun. It has a surface temperature of about 5836 K and is estimated to have an age of around 3.2 billion years. In comparison, the Sun is about 4.6 billion years old and has a surface temperature of 5778 K. With an apparent magnitude of 14.2, it is too faint to be seen with the naked eye.

Question: Verify the following claims with "True" or "False": There is a celestial body called 1101 Clematis and it has a temperature of 155 kelvins.
Answer: True