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 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: 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: 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-17b
Content:  Kepler-17b is a planet in the orbit of star Kepler-17, first observed by the Kepler spacecraft observatory in 2011. Kepler-17b is a gas giant nearly 2.45 times the mass of Jupiter, and is sometimes described as a "super-Jupiter". The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2229 K. The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 0°.
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: HD 205739
Content:  with a projected rotational velocity of 4 km/s. It has 1.3 times the mass of the Sun and 1.6 times the Sun's radius. The abundance of iron is 60% greater than in the Sun, suggesting a higher metallicity. The star is radiating 3.5 times the luminosity of the Sun from its photosphere at an effective temperature of 6,276 K. A Jupiter-like planet has been detected in an eccentric orbit around this star via Doppler spectroscopy. The eccentricity of 0.27 indicates that the orbit carries the body from 0.65 AU out to 1.14 AU between periastron and apastron. The maximum surface temperature of the planet is ~400 K, varying by 100 K over the course of an orbit. There is a data trend in the results which may point to an additional companion further from its star, but this will require a longer observation period to validate.
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: Kepler-10c
Content:  Kepler-10c is the outermost of the two known planets of Kepler-10, completing one orbit of the star every 45.29485 days at a distance of 0.2407 AU. The inner planet, Kepler-10b, is a rocky planet that orbits every ~0.8 days at a distance of 0.01684 AU. Kepler-10c's equilibrium temperature is estimated at 584 K, almost four times hotter than Jupiter's. The planet's orbital inclination is 89.65º, or almost edge-on with respect to Earth and to Kepler-10. Transits have been observed at points where Kepler-10c has crossed in front of its host star. Kepler-10c was originally thought to have a mass of 15–19 Earth masses. With a radius only 2.35 (2.31 to 2.44) times that of Earth (and so a volume 12–15 times that of Earth), it 
Title: Kepler-5b
Content:  Kepler-5b is a Hot Jupiter with a mass that is 2.114 times that of Jupiter and a radius of 1.431 times Jupiter's radius. This also means that Kepler-5b is not very dense. The planet's measured density is 0.894 grams/cm3, less than that of pure water and comparable only to the density of Saturn, which is approximately 0.69 grams/cm3. The planet has an equilibrium temperature of 1868 K, making it fifteen times hotter than Jupiter. Kepler-5b orbits its host star every 3.5485 days at a mean distance of 0.05064 AU. In addition, with an orbital inclination of 86.3º, Kepler-5b orbits Kepler-5 almost edge-on with respect to Earth. In comparison, planet Mercury orbits the Sun at a distance of 0.387 AU every 87.97 days. The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2169 K.

Question: Verify the following claims with "True" or "False": The temperature of a planet is 171.0 (kelvins) and it has an apoapsis of 511592000.0 kilometres.
Answer: True