Title: (523719) 2014 LM28
Content:   orbits the Sun at a distance of 16.8–538.9 AU once every 4631 years and 1 month (1,691,491 days; semi-major axis of 277.83 AU). Its orbit has an eccentricity of 0.94 and an inclination of 85° with respect to the ecliptic. The body's observation arc begins with its official discovery observation by Pan-STARRS at Haleakala Observatory in May 2013.
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: (16960) 1998 QS52
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 0.31–4.1 AU once every 3 years and 3 months (1,194 days; semi-major axis of 2.20 AU). Its orbit has an exceptionally high eccentricity of 0.86 and an inclination of 18° with respect to the ecliptic. The body's observation arc begins with a precovery taken at the Siding Spring Observatory in June 1983, more than 15 years prior to its official discovery observation at Socorro.
Title: 2020 SL1
Content:  orbits the Sun at an average distance of 2.52 AU once every 3.99 years. Its orbit has a high eccentricity of 0.64 and an inclination of 14° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.91 AU at perihelion to 4.1 AU at aphelion, crossing the orbits of Earth and Mars. Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU, is classified as an Apollo asteroid. Having a long observation arc over 12 years, the orbit of is well-defined with a condition code of 1. Although it is classified as a potentially hazardous asteroid due to its large size combined with its small minimum orbit intersection distance of 0.047 AU from Earth's orbital path, the asteroid will not make any close approaches within 0.1 AU over the next 200 years. The closest Earth encounter by in the last 200 years was on 10 July 1972, when it passed within 0.073 AU of Earth at closest approach.
Title: (523972) 1999 CW8
Content:   is an Apollo asteroid that crosses Earth's orbit. It orbits the Sun at a distance of 0.9–3.6 AU once every 3 years and 4 months (1,221 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.60 and an inclination of 34° with respect to the ecliptic. The asteroid never approaches Earth closer than 0.2 AU in the foreseeable future, but occasionally makes close approaches to Mars of 0.07 AU. It makes one such approach in 2073, at 0.067 AU, and another one in 2103, at 0.094 AU. Due to 's relatively high inclination, although it passes closer to the Sun than the Earth (0.9 AU), it never comes closer than 0.2 AU.
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: (527603) 2007 VJ305
Content:   orbits the Sun at a distance of 35.1–347 AU once every 2640 years and 11 months (964,601 days; semi-major axis of 191.1 AU). Its orbit has an exceptionally high eccentricity of 0.82 and an inclination of 12° with respect to the ecliptic. The body's observation arc begins with a precovery taken during the Sloan Digital Sky Survey at Apache Point in November 2000. It has a minimum orbital intersection distance with Neptune of 5.4 AU. It 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. These extreme trans-Neptunian objects (ETNOs) can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine.
Title: (523692) 2014 EZ51
Content:  orbits the Sun at a distance of 40.4–64.4 AU once every 379 years and 3 months (138,537 days; semi-major axis of 52.4 AU). Its orbit has an eccentricity of 0.23 and an inclination of 10 deg with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Haleakala in April 2010.
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: (523731) 2014 OK394
Content:  orbits the Sun at an average distance of 42.33 AU once every 275 years. Its orbit has an eccentricity of 0.16 and an inclination of 4° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 35.4 AU at perihelion to 49.3 AU at aphelion. is in a 3:5 mean-motion orbital resonance with Neptune; for every three orbits it makes, Neptune orbits five times. Its orbit has a minimum orbit intersection distance approximately 5.6 AU from Neptune's orbital path.

Question: Verify the following claims with "True" or "False": it has an apoapsis of 520906000.0 Kilometers and an average speed of 16.54 km/s!
Answer: True