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: Gliese 581e
Content:  minimum mass of 1.7 Earth masses, it is one of the least massive extrasolar planets discovered around a normal star, and relatively close in mass to Earth. It is also the exoplanet with the smallest accurate true mass known. At an orbital distance of just 0.03 AU from its parent star, however, it orbits further in than the habitable zone. It is unlikely to possess an atmosphere due to its high temperature and strong radiation from the star. Although scientists think it probably has a rocky surface similar to Earth, it is also likely to experience intense tidal heating similar to (and likely more intense than) that affecting Jupiter's moon Io. Gliese 581e completes an orbit around its parent star in approximately 3.15 days.
Title: 51 Eridani b
Content:  The planet has a mass at least 2.6, but not more than 11. Its radius is about 1.11 times the radius of Jupiter. It orbits 11.1 AU from its host star, and has an orbital period of roughly 10,000 days. The average temperature is 700 K, which is substantially hotter than the 130 K average temperature of Jupiter, the planet in the Solar System of closest size. It has the second strongest methane signature of any exoplanet, after GJ 504 b. This methane signature, along with the low luminosity of the object, should produce additional clues as to how 51 Eridani b was formed. Astronomers also detected the presence of water in the planet's spectrum. Atmospheric modeling favors a low surface gravity and a partly cloudy atmosphere.
Title: HD 87883
Content:  our Sun. It is radiating 32% of the luminosity of the Sun from its photosphere at an effective temperature of 4,980 K. In August 2009, this star was found to have a planet via the radial velocity method. The orbital solution shows it to be a Super-Jupiter body in an elliptical orbit with a period of 2754 days and a typical separation of 3.6 AU. A relatively high deviation on the model fit suggests there may be an additional planetary companion in a close, perturbing orbit of the star. The orbital parameters of the known planet does not preclude the existence of an Earth-mass planet with a dynamically-stable orbit in the habitable zone. Since its orbit is relatively face-on, its true mass deviates significantly from its minimum mass, and is.
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.
Title: WASP-5b
Content:  WASP-5b is an extrasolar planet orbiting the star WASP-5 located approximately 1000 light-years away in the constellation Phoenix. The planet's mass and radius indicate that it is a gas giant with a similar bulk composition to Jupiter. The small orbital distance of WASP-5 b around its star mean it belongs to a class of planets known as hot Jupiters. The equilibrium planetary temperature would be 1717 K, but measured in 2015 temperature was still much higher at 2500 K. Dayside temperature measured in 2020 was 2000 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 12.1°.
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: GSC 03949-00967
Content:  In 2011 a transiting hot Jupiter planet TrES-5 was detected. The host star was one of the faintest stars to which a planetary companion was detected by the transit method at the time of discovery. The planet’s equilibrium temperature is 1,480 K. An additional planet on a 4-day orbit in the system was suspected since 2018, but refuted in 2021. Another object on a wide orbit, either star or planet, is still suspected.
Title: HD 196885
Content:  the Sun and 1.45 times the Sun's radius. The metallicity of this star – what astronomers term the abundance of elements with higher atomic number than helium – is nearly double that in the Sun. It is radiating 2.7 times the luminosity of the Sun from its photosphere at an effective temperature of 6,340 K. In 2004, a planet was announced to be orbiting the star in a 386-day orbit. Follow-up work published in 2008 did not confirm the original candidate but instead found evidence of a planet in a 1326 days. This object has a minimum estimated mass at least three times that of the planet Jupiter. Perturbation by the secondary star in this system may have driven the planet into a high inclination orbit. The secondary, 
Title: Gliese 581
Content:  positive; however, in 2015, a reanalysis of the data suggested that it could still exist. The planet is thought to be tidally locked to its star. If the planet has a dense atmosphere, it may be able to circulate heat. The actual habitability of the planet depends on the composition of its surface and the atmosphere. It is thought to have temperatures around −37 to −11 °C (−35 to 10 °F). By comparison, Earth has an average surface temperature of 15 °C (59 °F)—while Mars has an average surface temperatures of about −63 °C (−81 °F). The planet has, according to Vogt, a "100%" chance of supporting life, but this is disputed.

Question: Verify the following claims with "True" or "False": The temperature of the planet is 5807 and its apoapsis is 511592000.0 km!
Answer: False