Title: 2016 PQ
Content:  orbits the Sun at a distance of 0.9–2.9 AU once every 2 years and 8 months (961 days). Its orbit has an eccentricity of 0.54 and an inclination of 3° with respect to the ecliptic.
Title: 2013 FS28
Content:   is 83 AU from the Sun with a 7 year observation arc. It orbits the Sun at a distance of roughly 36–240 AU once every 1600 years. Its orbit has a high eccentricity of 0.7 and an inclination of 13° with respect to the ecliptic. It has a minimum orbital intersection distance with Neptune of 9 AU. The body's observation arc begins with its first official observation in March 2013, using the 4-meter Blanco Telescope at Cerro Tololo Observatory. 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. Such extreme trans-Neptunian objects (ETNOs) can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine. It comes to perihelion (closest approach to the Sun) around December 2119.
Title: 238P/Read
Content:  Before it was discovered came to perihelion on 2005 July 27. When it was discovered on 2005 October 24, it showed vigorous cometary activity until 2005 December 27. Outgassing likely began at least 2 months before discovery. The activity of is much stronger than 133P/Elst-Pizarro and 176P/LINEAR. This may indicate that the impact assumed to have triggered 's activity occurred very recently. Observations of when it was inactive in 2007 suggests that it has a small nucleus only about 0.6 km in diameter. It came to perihelion on 2011 March 10 and 2016 October 22. It will next come to perihelion on 2022 June 5. was the target of a mission proposal in NASA's Discovery Program in the 2010s called Proteus, however it was not selected for further development. Discovery program's founding mission was to an asteroid, but it went to a Near-Earth asteroid. A mission to a main-belt asteroid was proposed in the 1990s (also see Deep Impact (spacecraft)).
Title: (15789) 1993 SC
Content:  (15789) 1993 SC is a trans-Neptunian object of the plutino class. The discovery was made in 1993 at the La Palma Observatory with the Isaac Newton Telescope. It was the second plutino to receive an MPC number. KBO's found in 1993 include: (15788) 1993 SB, (15789) 1993 SC, (181708) 1993 FW, and (385185) 1993 RO.
Title: Great Comet of 1819
Content:  Orbital elements for the comet were calculated by several astronomers. The orbit is classified as parabolic and is nearly perpendicular to Earth's orbital plane, with an inclination of 80°. It passed closest to the Earth on June 25 at a distance of 0.67 AU and closest to the Sun on June 28 at 0.34 AU. The orbit of the comet and its transit of the Sun were later analyzed by astronomer John Russell Hind. In 2016 the orbit was recalculated based on a total of 692 observations of the comet taken in 1819, with the resulting conclusion that the comet will not return for over 3,000 years and represents no threat to the Earth, and that Near Eastern records around 2550 BCE may be found to mention its earlier passage.
Title: (20161) 1996 TR66
Content:  It orbits the Sun at a distance of 28.6–66.6 AU once every 328 years and 8 months (120,032 days). Its orbit has an eccentricity of 0.40 and an inclination of 12° with respect to the ecliptic. Near perihelion, it comes closer to the Sun than Neptune does (29.7 AU). It has a semi-major axis (average distance from the Sun) near the edge of the classical belt.
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: 30P/Reinmuth
Content:  Comet 30P/Reinmuth, also known as Comet Reinmuth 1, is a periodic comet in the Solar System, first discovered by Karl Reinmuth (Landessternwarte Heidelberg-Königstuhl, Germany) on February 22, 1928. First calculations of orbit concluded a period of 25 years, but this was revised down to seven years and speculation this was the same comet as Comet Taylor, which had been lost since 1915. Further calculations by George van Biesbroeck concluded they were different comets. The 1935 approach was observed though not as favourable, in 1937 the comet passed close to Jupiter which increased the perihelion distance and orbital period. Due to miscalculations, the 1942 appearance was missed, but it has been observed on every subsequent appearance since. The comet nucleus is estimated to be 7.8 kilometers in diameter.
Title: 2830 Greenwich
Content:  Greenwich is a member of the Phocaea family (701), a group of asteroids with similar orbital characteristics. It orbits the Sun in the inner main-belt at a distance of 1.9–2.9 AU once every 3 years and 8 months (1,340 days). Its orbit has an eccentricity of 0.21 and an inclination of 25° with respect to the ecliptic. It was first identified as at Crimea-Nauchnij in 1969, extending the asteroid's observation arc by 11 years prior to its official discovery observation at Anderson Mesa.
Title: 2013 LX28
Content:  was discovered on 12 June 2013. As of September 2014, it has been observed 26 times with a data-arc span of 349 days. It is an Apollo asteroid and its semi-major axis (1.0016 AU) is very similar to that of the Earth but it has relatively high eccentricity (0.4521) and high orbital inclination (49.9761°). With an absolute magnitude of 21.7, it has a diameter in the range 130–300 m (for an assumed albedo range of 0.04–0.20).

Question: Verify the following claims with "True" or "False": The epoch of a planet (former name "1928 PC") is on 31 December 2016.
Answer: True