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: 2000 Herschel
Content:  Herschel is a member of the Phocaea family (701), a large family of stony asteroids with nearly two thousand known members. It orbits the Sun in the inner main-belt at a distance of 1.7–3.1 AU once every 3 years and 8 months (1,341 days; semi-major axis of 2.38 AU). Its orbit has an eccentricity of 0.30 and an inclination of 23° with respect to the ecliptic. It was first identified as at Johannesburg Observatory in 1934, extending the body's observation arc by 26 years prior to its official discovery observation at Sonneberg. The relatively high orbital eccentricity of this object causes it to come close to the orbit of the planet Mars. This means there is a chance it will eventually collide with the planet, with the odds of a collision estimated at 18% per billion orbits.
Title: ODERACS 2D
Content: COSPAR ID: 1995-004F ; SATCAT number: 23474 ; Mass: 1 kg ; Perigee: 314 km ; Apogee: 336 km ; Orbital period: 91 minutes ; Orbital inclination: 51.6° ; Eccentricity: 0.00164 ; Decay Date: March 2, 1995 
Title: 1240 Centenaria
Content:  Centenaria is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.4–3.4 AU once every 4 years and 10 months (1,773 days; semi-major axis of 2.87 AU). Its orbit has an eccentricity of 0.18 and an inclination of 10° with respect to the ecliptic. The asteroid was first observed as at the United States Naval Observatory in September 1915. The body's observation arc begins at Lowell Observatory in December 1930, or 14 months prior to its official discovery observation at Bergedorf.
Title: 1245 Calvinia
Content:  According to Zappalà, Mothé-Diniz, as well as Milani and Knežević, Calvinia is a member of the Koronis family (605), a very large outer asteroid family with nearly co-planar ecliptical orbits. Interestingly, in one of the most recent and complete synthetic HCM-analysis by Nesvorný, Calvinia is not a Koronian asteroid but belongs to the background population. It orbits the Sun in the outer main-belt at a distance of 2.7–3.1 AU once every 4 years and 11 months (1,796 days; semi-major axis of 2.89 AU). Its orbit has an eccentricity of 0.08 and an inclination of 3° with respect to the ecliptic. The asteroid was first observed as at the Heidelberg Observatory in March 1906. The body's observation arc begins with its official discovery observation at Johannesburg in May 1932.
Title: ODERACS 2C
Content: COSPAR ID: 1995-004E ; SATCAT number: 23473 ; Mass: 1 kg ; Perigee: 314 km ; Apogee: 336 km ; Orbital period: 91 minutes ; Orbital inclination: 51.6° ; Eccentricity: 0.00164 
Title: ODERACS 2A
Content: COSPAR ID: 1995-004C ; SATCAT number: 23471 ; Mass: 5 kg ; Perigee: 314 km ; Apogee: 336 km ; Orbital period: 91 minutes ; Orbital inclination: 51.6° ; Eccentricity: 0.00164 
Title: 2011 EO40
Content:  was discovered by Richard A. Kowalski on 10 March 2011 while observing for the Mount Lemmon Survey. Its orbit is typical of Apollo asteroids and is characterized by significant eccentricity (0.54), low inclination (3.36º), and a semi-major axis of 1.65 AU. Upon discovery, it was classified as an Earth crosser, a near-Earth asteroid (NEA) and a potentially hazardous asteroid (PHA) by the Minor Planet Center. It was listed on the Sentry Risk Table for less than one day. Its orbit is in need of additional observations to determine if it is part of an asteroid family; as of October 2015 the orbit is determined using just twenty observations spanning an observation arc of 34 days. has an absolute magnitude of 21.5, which gives a characteristic diameter of about 200 m.
Title: 302 Clarissa
Content:  Clarissa (minor planet designation: 302 Clarissa) is a typical main belt asteroid. The asteroid was discovered by the French astronomer Auguste Charlois on 14 November 1890 in Nice. The origin of the name is unknown. In 1991, 302 Clarissa was being considered as a possible fly-by target for the Cassini spacecraft, but was later removed from consideration. This body is orbiting the Sun with a period of 1362.5 days and an eccentricity (ovalness) of 0.11. The orbital plane is inclined by 3.4° to the plane of the ecliptic. There are no major planetary resonances near the orbit of 302 Clarissa. It has a retrograde spin with a rotation period of 14.4797 hours. Stellar occultation data provides a 
Title: 2349 Kurchenko
Content: Occultation Kurchenko is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.4–3.1 AU once every 4 years and 7 months (1,683 days; semi-major axis of 2.77 AU). Its orbit has an eccentricity of 0.12 and an inclination of 17° with respect to the ecliptic. The body's observation arc begins with its observation as at Goethe Link Observatory in November 1957, almost 13 years prior to its official discovery observation at Nauchnij. On 19 October 2008, the asteroid occulted the star. All five observers reported a negative result.

Question: Verify the following claims with "True" or "False": 100050 Carloshernandez has an epoch date of December 31st 2006 and a periapsis of 445895000000.0.
Answer: False