Title: 147 Protogeneia
Content:  Based upon its spectrum, it has a Tholen classification as a C-type asteroid, which indicates has a dark surface and probably a primitive composition of carbonaceous material. Photometric observations of this asteroid at the Altimira Observatory in 2004 gave a light curve with a period of 7.8528 ± 0.0008 hours and a brightness variation of 0.28 in magnitude. A photometric study was reported in 2006 from the Yunnan Observatory in China, finding a matching period of 7.852 hours and a brightness variation of 0.25 magnitude. They estimate the ratio of the lengths for the asteroid's major and minor axes is at least 1.26:1. There is one reported stellar occultation by Protogeneia, on May 28, 2002, from Texas.
Title: 147 Protogeneia
Content:  Protogeneia (minor planet designation: 147 Protogenia) is a large main belt asteroid that was discovered by Hungarian astronomer Lipót Schulhof on July 10, 1875, from the Vienna Observatory; it was his only asteroid discovery. Its name is Greek for "first born" and was chosen by Karl L. Littrow in allusion to the fact that this was the first asteroid discovered by an astronomer who was already known for work in other fields of astronomy. This object has a low orbital eccentricity and inclination. With an orbital period roughly double that of the planet Jupiter, it has been identified as a member of the Hecuba group of asteroids that share a 2:1 mean-motion orbital resonance with the giant 
Title: 147
Content: 147 Protogeneia, a large main belt asteroid with a low eccentricity and low inclination ; NGC 147, a Dwarf spheroidal galaxy about 2.58 million light-years away in the constellation Cassiopeia ; Promethium-147, an isotope of promethium with a half-life of 2.62 years ; JWH-147 is an analgesic drug used in scientific research, which acts as a cannabinoid agonist at both the CB1 and CB2 receptors 
Title: 147 (number)
Content: The year AD 147 or 147 BC ; 147 AH is a year in the Islamic calendar that corresponds to 764 &ndash; 765 CE ; 147 Protogeneia is a large main belt asteroid with a low eccentricity and low inclination ; NGC 147 (DDO3) is a Dwarf spheroidal galaxy about 2.58 million light-years away in the constellation Cassiopeia ; Promethium-147 is an isotope of promethium with a half-life of 2.62 years ; JWH-147 is an analgesic drug used in scientific research, which acts as a cannabinoid agonist at both the CB1 and CB2 receptors ; Sonnet 147 147 is also:
Title: 14 Arietis
Content:  14 Arietis (abbreviated 14 Ari) is a star in the constellation of Aries. 14 Arietis is the Flamsteed designation. It has an apparent visual magnitude of 4.98, which means it is visible to the naked eye. Based upon a measured annual parallax shift of 11.30 mas, is it located at a distance of approximately 290 ly, give or take a 30 light-year margin of error. This is an astrometric binary system. The primary has a stellar classification of F2 III, suggesting that it is a giant star. Despite being an evolved star with four times the radius of the Sun, it is spinning rapidly with a projected rotational velocity of 139.6 km/s. This is causing a pronounced equatorial bulge, with the radius of the star along the equator being 24% greater than the radius at the poles. The star shines at 32 times the luminosity of the Sun, with this energy being radiated from its outer atmosphere at an effective temperature of 6,761 K. This heat gives it the yellow-white hued glow of an F-type star.
Title: V1400 Centauri
Content:  1SWASP J140747.93−394542.6 (also known as 1SWASP J140747, J1407 and Mamajek's Object) is a star similar to the Sun in the constellation Centaurus at a distance of about 434 light years from Earth. A relatively young star, its age is estimated to be 16 million years, and its mass is about 90% that of the Sun. The star has an apparent magnitude of 12.3 and requires a telescope to be seen. The star's name comes from the SuperWASP (Wide Angle Search for Planets) program and the star's coordinates. The star is variable due to the planet orbiting around it and has been given the variable star designation V1400 Centauri. In 2007, J1407 was observed to be eclipsed and orbited by at least one major body, 1SWASP J1407b (J1407b), thought to be either a large gas giant planet or a brown dwarf with an immense ring system. Subsequent observations have not successfully detected J1407b, suggesting that it is on a highly eccentric orbit around the star. By 2021, it was discovered the parent star is strongly variable, with a 5.4-year long magnetic activity cycle.
Title: 14 Sagittarii
Content:  14 Sagittarii is a single, orange-hued star in the southern zodiac constellation of Sagittarius. It is faintly visible to the naked eye under good seeing conditions, having an apparent visual magnitude of 5.49. Based upon an annual parallax shift of 7.2 mas, it is located some 450 light years away. The star is moving closer to the Sun with a heliocentric radial velocity of around −59 km/s. It should achieve perihelion in about two million years, approaching as close as 41.72 pc. This is an evolved giant star with a stellar classification of K2 III, having exhausted the supply of hydrogen at its core and moved off the main sequence. It is a suspected variable star, possibly of the micro-variable variety, having an amplitude of less than 0.03 in magnitude. 14 Sagittarii is radiating about 317 times the Sun's luminosity from its photosphere at an effective temperature of around 3,940 K.
Title: 14 Sagittae
Content:  14 Sagittae is a binary star system in the equatorial constellation of Aquila. 14 Sagittae is the Flamsteed designation. It appears as a sixth magnitude star, near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 5.89. The system is located 660 light years away, as determined from its annual parallax shift of 4.91 mas. It is moving closer to the Earth with a heliocentric radial velocity of –22 km/s. This is a single-lined spectroscopic binary with an orbital period of 61.5 days and an eccentricity of 0.49. The visible component is a chemically peculiar mercury-manganese star with a stellar classification of B9p HgMn. It is narrow-lined with a projected rotational velocity of 7 km/s. The star is radiating 292 times the Sun's luminosity from its photosphere at an effective temperature of 13,200 K.
Title: Kepler-14
Content:  so close-knit as seen from Earth, it was impossible for the discovery team to separate the two stars and analyze their characteristics as separate stars. The Kepler team analyzed their characteristics under the assumption that Kepler-14 was a single star. If Kepler-14 were a single star, it would be an F-type star with a mass of 1.512 times the Sun's, and a size that is 2.048 times the Sun's radius. As a single star, the effective temperature of Kepler-14 would be 6395 K, much hotter than the Sun, and the star's iron content would be 0.12, or 132% the amount found in the Sun. Assuming that Kepler-14's two stars formed at about the same time, their gyrochronological ages would be approximately 2.2 billion years.
Title: K2-148b
Content:  K2-148b orbits a late-K dwarf star known as K2-148, or EPIC 220194974. It is 63% the radius, 65% the mass, and 10% the luminosity of the Sun, with a temperature of 4079 K and an unknown age. For comparison, the Sun has a temperature of 5778 K and is 4.5 billion years old. It is orbited by a slightly smaller M0.5V red dwarf known as EPIC 220194953 at a distance of 1,100 AU. The companion star is about 58% the radius, 60% the mass, and 6.6% as luminous as the Sun with a temperature of 3854 K. EPIC 220194953 is slightly more metal-rich than K2-148, and the two are confirmed to be gravitationally bound to each other.

Question: Verify the following claims with "True" or "False": The celestial body known as 147 Protogeneia has a temperature of 155 kelvins and an apoapsis of 520906000.0 Kilometers.
Answer: False