Title: (585310) 2017 YZ1
Content:   is a member of the Apollo asteroids, which cross the orbit of Earth. Apollo's are the largest group of near-Earth objects with nearly 10 thousand known objects. It orbits the Sun at a distance of 0.88–1.77 AU once every 18 months (558 days; semi-major axis of 1.33 AU). Its orbit has an eccentricity of 0.33 and an inclination of 21° with respect to the ecliptic.
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: 2015 BP513
Content:   (also written 2015 BP513) is an Apollo near-Earth asteroid roughly 12–27 meters in diameter that passed less than 1 lunar distance from Earth on 18 January 2015.
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: 2020 XL5
Content:  The orbit of is well-defined with an uncertainty parameter of 2 and observation arc of 348 days. Additional observations over several oppositions are necessary to constrain its orbit over the long-term. orbits the Sun at an average distance of 1.001 AU once every 365.8 days, or approximately 1 Earth year. Its orbit has a high eccentricity of 0.388 and an inclination of 13.8° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.61 AU at perihelion to 1.39 AU at aphelion, crossing the orbits of Venus and Earth. Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU (by a small margin), is classified as an Apollo asteroid.
Title: (523662) 2012 MU2
Content:   is a member of the Apollo asteroids, a group of near-Earth objects with an Earth-crossing orbit. It orbits the Sun at a distance of 1.0–3.1 AU once every 2 years and 11 months (1,076 days; semi-major axis of 2.06 AU). Its orbit has an eccentricity of 0.51 and an inclination of 11° with respect to the ecliptic. On 24 June 2012 with an observation arc of 6 days,  showed a 1 in 7,140 chance of impacting Earth on 1 June 2015. It was removed from the Sentry Risk Table on the next day (25 June). With an observation arc of 113 days, the JPL Small-Body Database (solution JPL 42 dated 2013-Aug-05) shows that  may make a very close approach to asteroid 29 Amphitrite on 8 April 2179. The minimum approach distance is about 0.000032 AU, but the maximum distance is 0.14 AU. The nominal approach is 0.047 AU. The Earth approach in 2015 occurred on 15 May 2015 at a distance of 0.11485 AU.
Title: 2019 PG1
Content:    belongs to the Apollo asteroids, which cross the orbit of Earth. Apollos are the largest group of near-Earth objects with about 10 thousand known members. It orbits the Sun at a distance of 0.999–3.92 AU once every 3 years and 10 months (1,407 days; semi-major axis of 2.46 AU). Its orbit has an eccentricity of 0.59 and an inclination of 20° with respect to the ecliptic. With an uncertainty parameter of 4 and 5, respectively, long term predictions of the object's trajectory are imprecise.  is also a potentially hazardous asteroid (PHA) because its minimum orbit intersection distance (MOID) is less than 0.05 AU and its diameter is greater than 150 meters. The Earth-MOID is 0.00697 AU.
Title: (523794) 2015 RR245
Content:  As of 2018, has a reasonably well defined orbit with an uncertainty of 3. It orbits the Sun at a distance of 33.8–128.6 AU once every 731 years and 6 months (for reference, Neptune's orbit is at 30 AU). Its orbit has an eccentricity of 0.58 and an inclination of 8° with respect to the ecliptic. is among the most distant known Solar System objects. As of 2018, it is 63 AU from the Sun. It will make its closest approach to the Sun in 2093, when it will reach an apparent magnitude of 21.2.
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: (523775) 2014 YB35
Content:  is a member of the Apollo asteroids, a group of near-Earth object with an Earth-crossing orbit. It orbits the Sun at a distance of 1.0–2.8 AU once every 2 years and 7 months (939 days; semi-major axis of 1.88 AU). Its orbit has an eccentricity of 0.48 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins at with its official discovery observation at Catalina Station in December 2014.

Question: Verify the following claims with "True" or "False": They say it has an apoapsis of 511592000.0 kilometres.
Answer: True