Title: 2006 RH120
Content:  is now in solar orbit as an Amor-class asteroid with an orbit completely outside of Earth's orbit. As of 2017, this object was 2 AU from Earth on the other side of the Sun. Systematic residuals in the positions of the object probably indicate that the model used to determine solar radiation pressure may be too simple to adequately describe its motion over a long period of time. The next near-Earth encounter is in August 2028 when the object will pass Earth at a relatively low speed of 136 m/s. For comparison, on 13 April 2029, asteroid 99942 Apophis will pass Earth at a relative speed of 7.4 km/s. is listed as part of the Near-Earth Object Human Space Flight Accessible Targets Study (NHATS).
Title: (111253) 2001 XU10
Content:  orbits the Sun at a distance of 0.98–2.52 AU once every 2 years and 4 months (848 days; semi-major axis of 1.75 AU). Its orbit has an eccentricity of 0.44 and an inclination of 42° with respect to the ecliptic. The body's observation arc begins with a precovery taken by the Sloan Digital Sky Survey in February 2000. is a member of the Apollo asteroids, the largest subgroup of near-Earth asteroids which cross the orbit of Earth. It is also a Mars-crosser, as it crosses the orbit of the Red Planet at 1.66 AU.
Title: 2013 TV135
Content:   is an Apollo near-Earth asteroid estimated to have a diameter of 450 m. On 16 September 2013, it passed about 0.0448 AU from Earth. On 20 September 2013, it came to perihelion (closest approach to the Sun). The asteroid was discovered on 12 October 2013 by Ukrainian amateur astronomer Gennadiy Borisov with a custom 0.2 m telescope using images dating back to 8 October 2013. It was rated level 1 on the Torino Scale from 16 October 2013 until JPL solution 26 on 3 November 2013. It was removed from the JPL Sentry Risk Table on 8 November 2013 using JPL solution 32 with an observation arc of 27 days.
Title: 2012 FP35
Content:   is an Apollo asteroid about 11 meters in diameter, that made some close approaches to Earth. It orbits the Sun every 583.2 days,  in an ellipse between 0.749 AU  and 1.983. It was discovered on March 24, 2012 by the Catalina Sky Survey. This asteroids was calculated to have passed roughly 0.22 AU from Earth on September 20, 2015. It came within 0.00107 AU of Earth on March 26, 2012. The asteroid is about 7–15 meters in diameter. The size of the asteroid is estimated from the absolute magnitude.
Title: (394130) 2006 HY51
Content:  orbits the Sun at a distance of 0.1–5.1 AU once every 4 years and 2 months (1,527 days). Its orbit has an eccentricity of 0.97 and an inclination of 33° with respect to the ecliptic. It is the asteroid with the third-smallest known perihelion of any known object orbiting the Sun. Its extreme orbital eccentricity brings it within 0.081 AU of the Sun (26% of Mercury's perihelion) and as far as 5.118 AU from the Sun (making it a Jupiter-grazer). It has a minimum orbit intersection distance with Earth of 0.1064 AU, equivalent to 41.5 lunar distances. The small bodies with even more eccentric orbits are likely to suffer a rotational breakup by the age comparable to that of the Solar System, although 2006 HY51 itself is not expected to break.
Title: (248835) 2006 SX368
Content:  Centaurs have short dynamical lives due to strong interactions with the giant planets. The orbit of  is unusually eccentric — near the perihelion it comes under influence of Uranus, while at the aphelion it travels slightly beyond the orbit of Neptune. It orbits the Sun at a distance of 11.9–32.0 AU once every 103 years and 2 months (37,683 days; semi-major axis of 22.0 AU). Its orbit has an eccentricity of 0.46 and an inclination of 36° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Apache Point in September 2006.
Title: (154276) 2002 SY50
Content:  is a member of the Earth-crossing group of Apollo asteroids, the largest group of near-Earth objects with approximately 10 thousand known members. It orbits the Sun at a distance of 0.53–2.88 AU once every 2 years and 3 months (813 days; semi-major axis of 1.7 AU). Its orbit has an eccentricity of 0.69 and an inclination of 9° with respect to the ecliptic. Due to its large aphelion of 2.88 AU, it also crosses the orbit of Mars at 1.66 AU. The body's observation arc begins one month prior to its official discovery observation with its first observation by the NEAT program at Palomar Observatory in August 2002.
Title: 2006 RH120
Content:  On 14 June 2007, made its fourth and last perigee of the most recent Earth encounter. It was 0.7 lunar distances at closest, with an apparent magnitude of 18.5–19.0. Astronomers at JPL Goldstone in California made radar astrometry measurements on 12, 14 and 17 June 2007.
Title: (394130) 2006 HY51
Content:   is a near-Earth object of the Apollo asteroid group with a high orbital eccentricity, approximately 1.2 kilometers in diameter. It was discovered on 26 April 2006, by LINEAR at Lincoln Lab's ETS in Socorro, New Mexico, United States.
Title: 2013 TV135
Content:  With an orbital inclination of only 6.7 degrees and perihelion 0.99 AU from the Sun, the point of perihelion is controlled by close approaches to Earth. With a short observation arc of 108 days, it has an orbit with an Uncertainty of 4. Given the relatively large size of the asteroid, astronomers were able to refine the orbit of this asteroid over several months.

Question: Verify the following claims with "True" or "False": A planet, with the epoch date December 31st 2006, has an apoapsis of 511592000.0 km and an orbital period of 135589000.0.
Answer: True