Title: Prognoz 9
Content: Mass: 1060 kg ; Periapsis: 380 km ; Apoapsis: 720000 km ; Period: 38448.0 min (26.7 days) ; Inclination: 65.5°.  The spacecraft with highly eccentric orbit was spin stabilized with a period of 113 s. The spin axis pointed towards the Sun, and was repointed every few days.
Title: 2021 AV7
Content:  With a long observation arc spanning over 4 years, the orbit of is well-secured with a condition code of 1. The earliest known precovery observations of are from Pan-STARRS 1 on 9 July 2016. These precovery observations were published by the Minor Planet Center on 30 April 2021. orbits the Sun at an average distance of 3.05 AU once every 5.33 years. Its orbit has a high eccentricity of 0.71 and an inclination of 29° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.90 AU at perihelion to 5.2 AU at aphelion, crossing the orbits of Earth, Mars, and Jupiter. Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU, is classified as an Apollo asteroid. Although its nominal orbit has a small minimum orbit intersection distance around 0.00047 AU from Earth's orbital path, the asteroid will not make any close approaches within 0.2 AU over the next 200 years.
Title: Expedition 7
Content: Perigee: 384 km ; Apogee: 396 km ; Inclination: 51.6° ; Period: 92 min 
Title: 2014 FZ71
Content:   orbits the Sun at a distance of 55.8–95.8 AU once every 660 years and 3 months (241,142 days; semi-major axis of 75.82 AU). Its orbit has a moderate eccentricity of 0.26 and an inclination of 26° with respect to the ecliptic. The object belongs to the same orbital group as ("Buffy"),,  and  (also see diagram). With an orbital period of 660 years, it seems to be resonant trans-Neptunian objects in a 1:4 resonance with Neptune, as are and, but with a lower eccentricity and therefore higher perihelion. Considered a scattered and detached object,  is particularly unusual as it has an unusually circular orbit for a scattered-disc 
Title: 2021 PH27
Content:   orbits the Sun at a distance of 0.13–0.79 AU once every 4 months (114 days; semi-major axis of 0.46 AU). Its orbit has an eccentricity of 0.71 and an inclination of 32 degrees with respect to the ecliptic. It is classified as a near-Earth object (NEO) due its perihelion distance being less than 1.3 AU. It also falls under the NEO category of Atira asteroids, whose orbits are confined entirely within Earth's orbit at 1 AU from the Sun. Its orbit crosses the paths of Mercury and Venus, with nominal minimum orbit intersection distances of 0.11 AU and 0.015 AU, respectively. , holds the record for the smallest semi-major axis (0.46 AU) and shortest orbital period (114 days) of any known asteroid, supplanting  and 594913 ʼAylóʼchaxnim (0.56 AU, 151 days). For comparison, Mercury has a semi-major axis of 0.39 
Title: 2017 YE5
Content:  orbits the Sun at an average distance of approximately 2.82 AU, taking 4.73 years to complete one orbit. The orbit of is slightly inclined to the ecliptic plane by 6.2 degrees, with its farthest apsis oriented below the ecliptic. has a highly elongated orbit with an orbital eccentricity of 0.71. Over the course of its orbit, approaches 0.82 AU from the Sun at perihelion and recedes 4.82 AU from the Sun at aphelion, beyond the outer extent of the asteroid belt. At aphelion, approaches close to Jupiter's orbit, with a minimum orbital intersection distance (MOID) of 0.42 AU. At such close proximity to Jupiter's orbit, has likely been gravitationally perturbed by Jupiter, 
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: 2018 RY7
Content:  The asteroid's orbit determination is in need of some improvement. It orbits the Sun at a distance of 0.87–1.17 AU once every 374 days (semi-major axis of 1.016 AU). Its orbit has an eccentricity of 0.1470 and an inclination of 13.35° with respect to the ecliptic. It is a member of Apollo dynamical class in both the JPL Small-Body Database and the Minor Planet Center. Apollo asteroids are Earth-crossing asteroids.
Title: 2012 FC71
Content:  is locked in a Kozai resonance and as such it has a very slow orbital evolution and it will remain relatively unperturbed for hundreds of thousands of years. It had a close encounter with the Earth on 18 April 2012 at 0.076 AU when it was discovered and another on 17 May 2013 at 0.0581 AU, which was not observed.
Title: 71 Tauri
Content:  71 Tauri is a suspected triple star system in the zodiac constellation Taurus, located 146 light years from the Sun. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of +4.48. The star is moving further away from the Earth with a heliocentric radial velocity of +38 km/s. It is a member of the Hyades open cluster. The primary component is an F-type main-sequence star with a stellar classification of F0 V. It is a Delta Scuti variable with an amplitude of 0.02 in magnitude and a frequency of 0.16 d−1. This star has about 1.94 times the mass of the Sun and 3.34 times the Sun's radius. It has a projected rotational velocity of 192 km s−1, for an estimated rotation period of 14.2 days. Extreme ultraviolet flares have been observed coming from this star's hot corona, and it is the second brightest X-ray source in the Hyades.

Question: Verify the following claims with "True" or "False": Its rotation period is 79218.0 and it's apoapsis is 511592000.0 kilometres.
Answer: False