Title: HD 146624
Content:  suspected to be chemically peculiar. It is a young star, just 10 million years old, with a projected rotational velocity of 39 km/s. The mass of the star is greater than the Sun's, with De Rosa et al. (2014) estimating 1.49 times the mass of the Sun, while Zorec and Royer (2012) gives a multiplier of 2.13. It has 1.60 times the Sun's radius and shines with 21 times the Sun's luminosity from its photosphere at an effective temperature of 9,441 K. The star displays an infrared excess, suggesting a circumstellar disk of orbiting material. This has a mean temperature of 280 K, matching a disk radius of 4.2 AU.
Title: HD 21447
Content:  HD 21447 is a probable binary star system located in the constellation Camelopardalis. The star is also known as HR 1046. It can be viewed with the naked eye, having an apparent visual magnitude of 5.09. Based upon an annual parallax shift of 16.42 mas, it is located some 199 light years from the Sun. It is a candidate for membership in the Ursa Major Moving Group. The primary component is A-type main-sequence star with a stellar classification of A1 Va. It is around 146 million years old and is spinning with a projected rotational velocity of 182 km/s. The star has an estimated 2.32 times the mass of the Sun and about 1.9 times the Sun's radius. It is radiating around 32 times the Sun's luminosity from its photosphere at an effective temperature of 10,049 K. The companion is visual magnitude 9.4 star at an angular separation of 14.8 arcsec.
Title: HD 219623
Content:  Sun. HD 219623 is around 1.2 billion years in age, with a projected rotational velocity of 5.5 km/s. Compared to the Sun, it has a slightly higher abundance of elements other than hydrogen and helium—what astronomers term the star's metallicity. The effective temperature of the stellar atmosphere is about 6,138 K, giving it the yellow-white hued glow of an ordinary F-type star. In 2006, this star was examined using the MIPS instrument on the Spitzer Space Telescope. An infrared excess at a wavelength of 70 μm was detected with 3-σ certainty. The data suggests the presence of circumstellar disk of orbiting dust, which is likely being replenished via debris from comets or asteroids. The temperature of this dust indicates the inner edge of the disk annulus comes to within 0.4 AU of the host star, while the outer edge extends out to around 22 AU.
Title: 21 Aquarii
Content:  21 Aquarii is a single star in the zodiac constellation of Aquarius. 21 Aquarii is the Flamsteed designation. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.49. This object is a member of the HR 1614 moving group, and is moving closer to the Earth with a heliocentric radial velocity of −24.5 km/s. This object is an evolved giant star with a stellar classification of K4 III. As a result of having exhausted the hydrogen at its core, it has expanded to 27 times the radius of the Sun. The star is radiating 203 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,120 K.
Title: HD 219623
Content:  HD 219623 is the Henry Draper Catalogue designation for a solitary star in the northern circumpolar constellation of Cassiopeia. It has an apparent visual magnitude of 5.59, which lies in the brightness range that is visible to the naked eye. According to the Bortle scale, it can be observed from dark suburban skies. Parallax measurements made by the Hipparcos spacecraft place it at an estimated distance of around 66.9 light years. It has a relatively high proper motion, advancing 262 milliarcseconds per year across the celestial sphere. This star has a stellar classification of F7 V, indicating that it is an F-type main-sequence star that is generating energy at its core through the thermonuclear fusion of hydrogen into helium. It is larger than the Sun, with 120% of the Sun's radius and 122% of the solar mass; as such, it shines nearly twice as brightly as 
Title: Sterope (star)
Content: 21 Tauri (or Sterope I, formally Asterope) ; 22 Tauri (or Sterope II)  The Sterope or Asterope  system is a double star in the zodiac constellation of Taurus. Its components have the Flamsteed designations 21 Tauri and 22 Tauri, and are sometimes known as Sterope I and Sterope II, respectively. The International Astronomical Union applies the name Asterope specifically to 21 Tauri. The two stars are thus  The two stars are separated by 0.047° on the sky, which is equal to 2.82 arc-minutes and thus closer than the usual naked-eye resolution limit of 4 arc-min, giving an elongated appearance of the two together. Both are members of the Pleiades open star cluster (M45) and approximately 440 light-years from the Sun.
Title: HD 1461
Content:  HD 1461 is a star in the equatorial constellation of Cetus, near the western constellation border with Aquarius. It has the Gould designation 32 G. Ceti, while HD 1461 is the Henry Draper Catalogue identifier. This object has a yellow hue and is a challenge to view with the naked eye, having an apparent visual magnitude of 6.47. The star is located at a distance of 76.5 ly from the Sun based on parallax, but is drifting closer with a radial velocity of −10 km/s. This object is a G-type main-sequence star with a stellar classification of G3VFe0.5, where the suffix notation indicates a mild overabundance of iron. It is roughly two billion years old and is spinning with a projected rotational velocity of 5 km/s. This is a solar-type star with 5% greater mass compared to the Sun and 1.24 times the Sun's radius. The star is radiating 1.19 times the luminosity of the Sun from its photosphere at an effective temperature of 5,386 K.
Title: 2101 Adonis
Content:  The near-Earth object orbits the Sun at a distance of 0.4–3.3 AU once every 2 years and 7 months (937 days; semi-major axis of 1.87 AU). Its orbit has an eccentricity of 0.76 and an inclination of 1° with respect to the ecliptic. Adonis was one of the first near-Earth objects ever to be discovered. It was also the second known Apollo asteroid after 1862 Apollo, the group's namesake discovered four years earlier in 1932.
Title: HD 216446
Content:  that the star has exhausted the supply of hydrogen at its core, then cooled and expanded off the main sequence. At present it has 25 times the radius of the Sun. The star has a lower abundance of elements other than hydrogen and helium compared to the Sun; what astronomers term the star's metallicity. It is radiating 193 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4288 K. The secondary companion, component B, is a magnitude 9.60 star located at an angular separation of 3.5 arcsecond from the primary, along a position angle of 38°, as of 1992.
Title: HD 6114
Content:  HD 6114 is a visual binary star system in the northern constellation of Andromeda. With a combined apparent magnitude of 6.46, the star can only be seen with the naked eye by keen-eyed observers even on the best of nights. Based upon an annual parallax shift of 10.4 mas as seen from Earth's orbit, the system is located approximately 96 pc distant. The binary nature of this system was discovered by O. Struve in 1864. It consists of a magnitude 6.76 primary component with a dimmer magnitude 8.07 secondary. As of 2015 the pair had an angular separation of 1.3 arcsecond along a position angle of 175°. The two stars orbit each other with a period of 450 years with an eccentricity of 0.80. The primary is an A-type main-sequence star with a stellar classification of A9 V. At the estimated age of 863 million years, it is spinning rapidly with a projected rotational velocity of 149 km/s. The star has 1.65 times the mass of the Sun and is radiating 21 times the Sun's luminosity from its photosphere at an effective temperature of 7,611 K.

Question: Verify the following claims with "True" or "False": The celestial body known as 2146 Stentor has a temperature of 171 kelvins and an apoapsis of 511592000 kilometres.
Answer: False