Title: HD 179070
Content:  The single known planet orbiting this star was identified as a candidate based on photometry from the first four months of data from the Kepler spacecraft. Confirmation was obtained in 2012 after extensive follow-up observations and analysis of the Kepler light curves. The calculated density of the planet is approximately 6.4 g cm−3, similar to earth's 5.5 g cm−3, which suggests a rocky composition. With an equilibrium temperature of 2025 Kelvin, the top few-hundred kilometers of the planet is probably molten.
Title: HD 171028
Content:  a projected rotational velocity of 2.3 km/s. It has the same mass as the Sun, but the radius is 2.4 times larger. The star is radiating 5.4 times the luminosity of the Sun from its photosphere at an effective temperature of 5,671 K. In the summer of 2007, a Jovian planetary companion was discovered by the HARPS planet search program using the radial velocity method. This object is orbiting at a distance of 1.32 AU from the host star with a period of 550 days and an eccentricity (ovalness) of 0.59. Since the inclination of the orbit is unknown, only a minimum mass can be determined. This planet has at least double the mass of Jupiter.
Title: HD 175167
Content:  It is radiating 2.9 times the Sun's luminosity from its photosphere at an effective temperature of 5,635 K. A Jovian planetary companion was discovered in 2010 by a team of the Magellan Planet Search Program, led by Pamela Arriagada. Designated HD 175167 b, their Doppler velocity data (taken over a five year period) indicates the planet has an orbital period of 1290 days at a distance of 2.40 AU from the host star with an eccentricity (ovalness) of 0.54. Since the inclination of the orbital plane is unknown, it is only possible to deduce a lower bound on the planet's mass. It is at least 7.8 times as massive as Jupiter. In a 2013 paper, Robert A. Wittenmyer and colleagues reviewed the data of this and many other systems with one or two planets for possible additional planets, but were unable to find any evidence of any.
Title: HIP 11915 b
Content:  HIP 11915 b is a jovian planet, an exoplanet with a mass and radius close to that of the planet Jupiter. It has a mass of 0.99 (315 ) and a likely radius of around 1. Based on models, it is expected to have a temperature of around 118 K. This is nearly the same as the planet Jupiter.
Title: Kepler-419c
Content:  Kepler-419c is a super-Jupiter, an exoplanet that has a radius and mass greater than that of the planet Jupiter. It has a temperature of 250 K, somewhat cooler than the equilibrium temperature of the Earth. It has a mass of 7.2, and a likely radius of around 1.13 , based on its high mass.
Title: 51 Pegasi b
Content:  are revising their theories of planet formation to account for them by studying orbital migration. Assuming the planet is perfectly grey with no greenhouse or tidal effects, and a Bond albedo of 0.1, the temperature would be 1265 K. This is between the predicted temperatures of HD 189733 b and HD 209458 b (1180 K–1392 K), before they were measured. In the report of the discovery, it was initially speculated that 51 Pegasi b was the stripped core of a brown dwarf of a decomposed star and was therefore composed of heavy elements, but it is now believed to be a gas giant. It is sufficiently massive that its thick atmosphere 
Title: TRAPPIST-1
Content:  TRAPPIST-1b has a semi-major axis of 0.012 AU and orbits its star every 1.51 day. It is also close enough to TRAPPIST-1 to be tidally locked. Trappist-1b is not within the habitable zone; it receives about 4 times as much irradiation as Earth and thus either was or still is a runaway greenhouse. It could have a thick atmosphere like Venus or lack one altogether like Mercury and, based on fluid dynamical arguments, is only slightly more likely than Earth to lack surface temperature gradients. Based on numerous climate models, the planet would have been desiccated by TRAPPIST-1's stellar wind and radiation although density estimates of the planet, if confirmed, demonstrate that it is not dense enough to consist solely of rock. Water could persist only in specific settings on the planet. Based on the Lyman-alpha radiation emissions, TRAPPIST-1b may be losing hydrogen at a rate of 46,000,000 g/s. It is also a candidate magma ocean planet.
Title: HD 231701
Content:  Babylonian civilizations in Mesopotamia. This object is an ordinary F-type main-sequence star with a stellar classification of F8 V. It is around three to 4.5 billion years old and may be evolving onto the subgiant branch. It is spinning with a projected rotational velocity of 4 km/s and has low chromospheric activity. HD 231701 has 1.2 times the mass of the Sun and 1.45 times the Sun's radius. It is radiating 2.6 times the luminosity of the Sun from its photosphere at an effective temperature of 6,081 K. In 2007, the N2K Consortium used the radial velocity technique to discover a Jupiter-like planet orbiting at a distance of 0.57 AU from the star with a period of 141.6 days.
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: Kepler-11b
Content:  Kepler-11b is estimated to be 2.78 Earth masses and 1.8 Earth radii, making it around three times (or less) as massive and nearly twice as large as Earth. The mass is determined using transit timing variations of Kepler-11c, and is limited by the quality of the data. Kepler-11b is the closest planet to its host star in the Kepler-11 planetary system. With an estimated density of 4.5 g/cm3, less than Venus's, Kepler-11b is denser than the solar system's gas giants but slightly less dense than the terrestrial planets. Early estimates have suggested that it is not of Earth-like composition, yet it is nonetheless composed mostly of elements heavier than helium. The planet's effective temperature is 900 K, and is thus the hottest of the planets discovered in the Kepler-11 system. Kepler-11b orbits its host star every 10.30375 days at a distance of .091 AU. Planet Mercury, in comparison, orbits the Sun every 87.97 days from a distance of .387 AU. Kepler-11b's inclination of 88.5° means that it deviates slightly from the orbital plane, but it does so more than the other five planets with which Kepler-11b was discovered.

Question: Verify the following claims with "True" or "False": The temperature of a planet is 171.0 (kelvins),has an escape velocity of 0.0112 kilometres per second and its apoapsis is 511592000.0 km.
Answer: True