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: 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: 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: 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: 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: 2MASS J01225093−2439505
Content:  In 2013, one superjovian planet (may be a brown dwarf), named 2MASS J01225093−2439505 b, was discovered by direct imaging. The measured planetary temperature is 1600 K, and it exhibits an unusual, short-lived atmospheric dust type due to its relatively low surface gravity and young age. The planetary spectrum is classified as L3.7. The planetary rotation axis is inclined to its orbit, obliquity is 33°, while the orbit is well aligned with the equatorial plane of the star, misalignment is 1°. The planet is rotating rapidly, with a period of 6.8 hours.
Title: K2-315b
Content:  The planet is thought to be a small rocky planet, even though composition is unknown. Since it orbits very close to its star, it is too hot to host life, due to it having a scorching temperature of 450 K. Not much is known about it because it was just discovered, but it is similar to Earth, having a radius 95% that of Earth, very similar to Venus, but has 81% Earth's mass.
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.
Title: 51 Pegasi b
Content:  After its discovery, many teams confirmed the planet's existence and obtained more observations of its properties. It was discovered that the planet orbits the star in around four days. It is much closer to it than Mercury is to the Sun, moves at an orbital speed of 136 km/s, yet has a minimum mass about half that of Jupiter (about 150 times that of the Earth). At the time, the presence of a huge world so close to its star was not compatible with theories of planet formation and was considered an anomaly. However, since then, numerous other "hot Jupiters" have been discovered (such as 55 Cancri and τ Boötis), and 

Question: Verify the following claims with "True" or "False": The celestial body known as a planet has a temperature of 171 kelvins, an escape velocity of 0.0112 kilometres per second and an apoapsis of 511592000.0 km.
Answer: True