Title: 2017 YE5
Content:  orbits the Sun at an average distance of approximately 2.82 AU, taking 4.73 years to complete one orbit. The orbit of is slightly inclined to the ecliptic plane by 6.2 degrees, with its farthest apsis oriented below the ecliptic. has a highly elongated orbit with an orbital eccentricity of 0.71. Over the course of its orbit, approaches 0.82 AU from the Sun at perihelion and recedes 4.82 AU from the Sun at aphelion, beyond the outer extent of the asteroid belt. At aphelion, approaches close to Jupiter's orbit, with a minimum orbital intersection distance (MOID) of 0.42 AU. At such close proximity to Jupiter's orbit, has likely been gravitationally perturbed by Jupiter, 
Title: 2021 AV7
Content:  With a long observation arc spanning over 4 years, the orbit of is well-secured with a condition code of 1. The earliest known precovery observations of are from Pan-STARRS 1 on 9 July 2016. These precovery observations were published by the Minor Planet Center on 30 April 2021. orbits the Sun at an average distance of 3.05 AU once every 5.33 years. Its orbit has a high eccentricity of 0.71 and an inclination of 29° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.90 AU at perihelion to 5.2 AU at aphelion, crossing the orbits of Earth, Mars, and Jupiter. Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU, is classified as an Apollo asteroid. Although its nominal orbit has a small minimum orbit intersection distance around 0.00047 AU from Earth's orbital path, the asteroid will not make any close approaches within 0.2 AU over the next 200 years.
Title: 2010 EU65
Content:  Sun at a distance of 17.0–22.9 AU once every 89 years and 3 months (32,606 days; semi-major axis of 19.97 AU). Its orbit has an eccentricity of 0.15 and an inclination of 15° with respect to the ecliptic. It has a Tisserand's parameter with respect to Jupiter (TJ) of 2.94, near the threshold of 3, typically used to distinguish asteroids from Jupiter-family comets. On 21 June 2021, the object came to perihelion at 17.0 AU and has since been moving away from the Sun. the object is at 17.009 AU, with a apparent magnitude of 21.71. The body's observation arc begins with a precovery observation taken by the Mount Lemmon Survey in April 2009.
Title: 514107 Kaʻepaokaʻawela
Content:   Kaʻepaokaʻawela orbits the Sun at a distance of 3.2–7.1 AU once every 11 years and 8 months (4,256 days; semi-major axis of 5.14 AU). Its orbit has an eccentricity of 0.38 and an inclination of 163° with respect to the ecliptic. Its period is close to the 11.86-year period of Jupiter. During one Jovian year, Jupiter moves 360° around the sun whereas Kaʻepaokaʻawela moves 366.3° in the opposite direction. The eccentricity of its orbit allows it to alternately pass inside and outside of Jupiter's orbit at its closest approaches of 176 million kilometers. Each time it passes near Jupiter its 
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: 2101 Adonis
Content:  The near-Earth object orbits the Sun at a distance of 0.4–3.3 AU once every 2 years and 7 months (937 days; semi-major axis of 1.87 AU). Its orbit has an eccentricity of 0.76 and an inclination of 1° with respect to the ecliptic. Adonis was one of the first near-Earth objects ever to be discovered. It was also the second known Apollo asteroid after 1862 Apollo, the group's namesake discovered four years earlier in 1932.
Title: Apsis
Content:  Currently, the Earth reaches perihelion in early January, approximately 14 days after the December solstice. At perihelion, the Earth's center is about 0.983 astronomical units (AU) or 147098070 km from the Sun's center. In contrast, the Earth reaches aphelion currently in early July, approximately 14 days after the June solstice. The aphelion distance between the Earth's and Sun's centers is currently about 1.017 AU or 152097700 km. The dates of perihelion and aphelion change over time due to precession and other orbital factors, which follow cyclical patterns known as Milankovitch cycles. In the short term, such dates can vary up to 2 days from one year to another. This significant 
Title: 2017 BS5
Content:  has a low-eccentricity orbit with a semi-major axis only slightly larger than that of Earth. It orbits the Sun at a distance of 1.008–1.023 AU once every 1.02 years (374 days). Its orbit has an eccentricity of 0.01 and an inclination of 11° with respect to the ecliptic. It has an Earth minimum orbital intersection distance of 0.007 AU, which corresponds to 2.7 lunar distances. The body is too small to be classified as a potentially hazardous asteroid.
Title: 3200 Phaethon
Content:  Phaethon is categorized as an Apollo asteroid, as its orbital semi-major axis is greater than that of the Earth's at 1.27 AU. It is also suspected to be a member of the Pallas family of asteroids. Its most remarkable distinction is that it approaches the Sun closer than any other named asteroid: its perihelion is only 0.14 AU &mdash; less than half of Mercury's perihelial distance. It is a Mercury-, Venus-, Earth-, and Mars-crosser as a result of its high orbital eccentricity. The surface temperature at perihelion could reach around 1025 K. Phaethon is a possible candidate for detecting general relativistic and/or solar oblateness effects in its orbital motion due to the frequent close approaches to the Sun. The Apollo asteroids (155140) 2005 UD and (225416) 1999 YC share similar orbits with Phaethon, suggesting a possible common breakup origin.
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": It has temperature of 171 kelvins and an apoapsis of 511592000 kilometres.
Answer: True