Title: 9950 ESA
Content:   ESA is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. It orbits the Sun at a distance of 1.1–3.7 AU once every 3 years and 10 months (1,390 days). Its orbit has an eccentricity of 0.53 and an inclination of 15° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Caussols in November 1990.
Title: 9950 ESA
Content:  9950 ESA, provisional designation, is an eccentric asteroid and elongated near-Earth object of the Amor group, approximately 1.7 kilometers in diameter. It was discovered on 8 November 1990, by French astronomer Christian Pollas at the Centre de recherches en géodynamique et astrométrie (Cerga) at Caussols in southeastern France. It was named for the European Space Agency (ESA).
Title: 9950 ESA
Content:  ESA has an Earth minimum orbit intersection distance of 0.2806 AU, which corresponds to 109.3 lunar distances. It approached the Earth at 0.393 AU on 18 October 1990, three weeks prior to its discovery, and made two more close approaches in August and September 2013, respectively. Its next close encounter with Earth will be in October 2032, at distance of 0.3043 AU. The eccentric asteroid is also a Mars-crosser. In March 1987, it approached the Red Planet at 0.0990 AU.
Title: 2005 RH52
Content:   belongs to a small group of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more. Such extreme trans-Neptunian objects (ETNOs) can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine. It orbits the Sun at a distance of 39–270 AU once every 1923 years and 10 months (702,689 days; semi-major axis of 154.68 AU). Its orbit has an eccentricity of 0.75 and an inclination of 20° with respect to the ecliptic. The body's observation arc begins with its first official observation at Mauna Kea in September 2005.
Title: ODERACS 2E
Content: COSPAR ID: 1995-004G ; SATCAT number: 23475 ; Mass: 5 kg ; Perigee: 314 km ; Apogee: 336 km ; Orbital period: 91 minutes ; Orbital inclination: 51.6° ; Eccentricity: 0.00164 ; Decay Date: February 27, 1995 
Title: 1995 GJ
Content:  The nominal orbit of 1995 GJ suggests it orbits the Sun at a distance of 39–46 AU once every 281 years with an assumed eccentricity of 0.09 and an inclination of 23° with respect to the ecliptic. But 1995 GJ has the highest possible orbital uncertainty and thus very large uncertainties in the orbital elements. With only a 1-day observation arc, the orbit is so poorly constrained as to be almost worthless. The eccentricity is listed as, even though realistically it will be less than 1. Otherwise known for their low inclinations, this cubewano may be the first of its kind to have an inclination greater than 20°. But as a 
Title: Planet Nine
Content: semi-major axis of 400–500 AU; ; orbital eccentricity of 0.15–0.3; ; orbital inclination around 20°; ; mass of about 5 Earth masses. In February 2019, the total of ETNOs that fit the original hypothesis of having semi-major axis of over 250 AU had increased to 14 objects. The orbit parameters for Planet Nine favored by Batygin and Brown after an analysis using these objects were: 
Title: (5645) 1990 SP
Content:  The asteroid orbits the Sun at a distance of 0.8–1.9 AU once every 1 years and 7 months (576 days). Its orbit has an eccentricity of 0.39 and an inclination of 14° with respect to the ecliptic.
Title: (90075) 2002 VU94
Content:  is a member of the dynamical Apollo group, which are Earth-crossing asteroids. Apollo asteroids are the largest subgroup of near-Earth objects. It orbits the Sun at a distance of 0.9–3.4 AU once every 3 years and 1 month (1,138 days; semi-major axis of 2.13 AU). Its orbit has an eccentricity of 0.58 and an inclination of 9° with respect to the ecliptic. The body's observation arc begins with a precovery from the Digitized Sky Survey taken at the Palomar Observatory in October 1955, or 47 years prior to its official discovery observation.
Title: (529366) 2009 WM1
Content:  orbits the Sun at a distance of 0.98–1.38 AU once every 15 months (468 days; semi-major axis of 1.18 AU). Its orbit has an eccentricity of 0.17 and an inclination of 26° with respect to the ecliptic. Even though has an Earth MOID of 0.00009 AU, the orbit and future close approaches are well determined with an orbital uncertainty of 1. On 23 November 2059, will pass 0.0046 AU from Earth. On 23 November 2199, it will make another close approach at a distance of 0.0005 AU to 0.069 AU, but since it is a close approach and the exact distance in uncertain, future close approaches after 2199 are uncertain.

Question: Verify the following claims with "True" or "False": 99950 Euchenor has a mass of 5.7 kilograms and an apoapsis of 520906000.0 km.
Answer: False