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-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: 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: 51 Orionis
Content:  51 Orionis is a single star in the equatorial constellation of Orion. It has the Bayer designation b Orionis, while 51 Orionis is the Flamsteed designation. This object is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.90. It is located approximately 299 light-years away from the Sun based on parallax, and is drifting further away with a radial velocity of +88 km/s. This is an aging giant star with a stellar classification of K1III, having exhausted the supply of hydrogen at its core and expanded to 19 times the Sun's radius. It is four billion years old with 1.11 times the mass of the Sun. The star is radiating 132 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,458 K.
Title: KELT-18b
Content:  KELT-18b has 1.18 times Jupiter's mass, and is 57% larger than Jupiter. Despite the high mass, its density is lower than Saturn's, and has a high equilibrium temperature of 2,085 K due to orbiting close to a hot star. The planet orbits at a distance 10 times closer than Mercury's in almost 3 days.
Title: KELT-9b
Content:  KELT-9b is a relatively large giant planet at about 2.8 times the mass of Jupiter; however, given that its radius is nearly twice that of Jupiter, its density is less than half that of Jupiter. Like many hot Jupiters, KELT-9b is tidally locked with its host star. The outer boundary of its atmosphere nearly reaches its Roche lobe, implying that the planet is experiencing rapid atmospheric escape driven by the extreme amount of radiation it receives from its host star. In 2020, atmospheric loss rate was measured to be equal to 18 - 68 Earth masses per billion years. As of January 2020, KELT-9b is one of the hottest known exoplanets, with dayside temperatures 
Title: TRAPPIST-1b
Content:  TRAPPIST-1b is very similar in both mass, radius, and gravity to Earth. It has a radius of 1.121, a mass of 1.02 , and about 81% Earth's surface gravity. However, the density of the planet indicates that it is not entirely rocky. With a density of 3.98 g/cm3, about ≤5% of its mass must be water, likely in the form of a thick Venus-like atmosphere due to it receiving being nearly four times more energy than Earth does. The planet's surface temperature is estimated to be between 750 K and 1500 K, potentially as high as 2000 K. This is much hotter than the surface of Venus and may be hot enough that the surface is molten lava.
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: 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: 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.

Question: Verify the following claims with "True" or "False": The temperature of a planet is 18100 (kelvins),has an escape velocity of 0.0112 kilometres per second and its apoapsis is 511592000.0 km.
Answer: False