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: 2020 AP1
Content:   is an Apollo near-Earth object roughly 5 m in diameter. On 2 January 2020 it passed 0.00218 AU from Earth. With a short 1-day observation arc it is roughly expected to pass about 0.01 AU from Earth on 7 January 2022, but with an uncertainty of ±8 days for the close approach date it could pass significantly closer or further.
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: 99942 Apophis
Content:  Apophis has a low inclination orbit (3.3°) that varies from just outside the orbit of Venus (0.746 AU) to just outside the orbit of Earth (1.099 AU). After the 2029 Earth approach the orbit will vary from just inside of Earth's to just inside of Mars.
Title: (5604) 1992 FE
Content:  (327 days) | mean_anomaly   = 286.36° | mean_motion    = {{Deg2DMS|1.1011|sup=ms}} / day | inclination    = 4.7136° | asc_node       = 311.96° | arg_peri       = 82.586° | moid           = 0.0332 AU{{·}}12.9 LD | venus_moid     = 0.0059 AU | mean_diameter   = 550 m  | rotation        = {{Convert|5.3375|h|d|abbr=on|lk=on}}} | albedo         = 0.48 | abs_magnitude  = 17.1 }} (5604) 1992 FE is an Aten-type near-Earth minor planet. It was discovered by Robert H. McNaught at the Siding Spring Observatory in Canberra, Australia, on March 26, 1992. The asteroid is 550 m in diameter. The asteroid has a Venus minimum orbit intersection distance (Venus–MOID) of 0.0059 AU. On April 7, 2015 the asteroid passed 0.00717 AU from Venus.
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: 2006 QQ23
Content:  On 10 August 2019 at 7:23 am UTC, safely passed 0.04977 au from Earth; travelling at around 4.67 km/s The asteroid was recovered on 14 July 2019, which extended the observation arc from 8 years to 12 years, and therefore it had a very small uncertainty in the 2019 approach. The uncertainty region in the close approach was ±60 km.
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: (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: 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.

Question: Verify the following claims with "True" or "False": A planet, with an escape velocity of 0.02 kmps, has an apoapsis of 520906000.0 (kilometres).
Answer: True