Title: 2016 EU85
Content:  orbits the Sun at a distance of 1.0–2.7 AU once every 2 years and 6 months (918 days). Its orbit has an eccentricity of 0.48 and an inclination of 3° with respect to the ecliptic. It has an Earth minimum orbital intersection distance of 0.0065 AU which translates into 2.5 lunar distances.
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: 2016 AZ8
Content:  orbits the Sun at a distance of 0.85–1.8 AU once every 18 months (554 days; semi-major axis of 1.32 AU). Its orbit has an eccentricity of 0.36 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins with a precovery taken at the Siding Spring Survey in July 2012, more than three years prior to its official discovery observation.
Title: Apsis
Content:  Orbital elements such as the time of perihelion passage are defined at the epoch chosen using an unperturbed two-body solution that does not account for the n-body problem. To get an accurate time of perihelion passage you need to use an epoch close to the perihelion passage. For example, using an epoch of 1996, Comet Hale–Bopp shows perihelion on 1 April 1997. Using an epoch of 2008 shows a less accurate perihelion date of 30 March 1997. Short-period comets can be even more sensitive to the epoch selected. Using an epoch of 2005 shows 101P/Chernykh coming to perihelion on 25 December 2005, but using an epoch of 2012 produces a less accurate unperturbed perihelion date of 20 January 2006. Numerical integration shows dwarf planet Eris will come to perihelion around December 2257. Using an epoch of 2021, which is 236 years early, less accurately shows Eris coming to perihelion is 2260. 4 Vesta comes to perihelion on 26 December 2021, but using a two-body solution at an epoch of July 2021 less accurately shows Vesta coming to perihelion on 25 December 2021.
Title: 13P/Olbers
Content:  13P/Olbers is a periodic comet with an orbital period of 69 years. It fits the classical definition of a Halley-type comet with (20 years < period < 200 years). Heinrich Wilhelm Matthias Olbers (Bremen) discovered the comet on March 6, 1815. Its orbit was first computed by Carl Friedrich Gauss on March 31, Friedrich Bessel calculated an orbital period as 73 years, later as 73.9 years, calculations by other astronomers during that era resulted anywhere between 72 and 77 years. The comet was last detected in 1956. It will next come to perihelion on June 30, 2024. the comet will be closest to the Earth on January 10, 2094 when it passes at a distance of 0.756 AU. There is some speculation that 13P/Olbers has an associated meteor shower on Mars coming from the direction of Beta Canis Major.
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: 2013 TV135
Content:  With an orbital inclination of only 6.7 degrees and perihelion 0.99 AU from the Sun, the point of perihelion is controlled by close approaches to Earth. With a short observation arc of 108 days, it has an orbit with an Uncertainty of 4. Given the relatively large size of the asteroid, astronomers were able to refine the orbit of this asteroid over several months.
Title: 2016 DV1
Content:   orbits the Sun at a distance of 0.7–3.0 AU once every 2 years and 6 months (913 days; semi-major axis of 1.84 AU). Its orbit has a high eccentricity of 0.63 and an inclination of 3° with respect to the ecliptic. It has an Earth minimum orbital intersection distance of 0.001 AU. Due to its eccentric orbit,  is also a Mars-crosser, crossing the orbit of the Red Planet at 1.66 AU.
Title: 2016 WF9
Content:  When was first announced and had a short insignificant 3 day observation arc, it was estimated to have a 7.6 year orbital period. The preliminary orbit was also listed on the JPL Sentry Risk Table, but none of the virtual impact dates were before 2029. As the observation arc became longer and the orbital parameters better constrained, it was removed from the Sentry Risk Table on 20 December 2016. With a 111-day observation arc, it is now known that it has a 4.86 year orbital period and currently stays inside the orbit of Jupiter. A simulation of 's dynamics over a period of 100 million days (~274,000 years) found that it had roughly a 60% chance of originating from the outer solar system as a long-period comet. 
Title: Equation of time
Content:  and D is the number of days past that epoch. At periapsis M = 2π , so solving gives D = Dp = 2.508. This puts the periapsis on 4 January 2000 at 00:11:41 while the actual periapsis is, according to results from the Multiyear Interactive Computer Almanac (abbreviated as MICA), on 3 January 2000 at 05:17:30. This large discrepancy happens because the difference between the orbital radius at the two locations is only 1 part in a million; in other words, radius is a very weak function of time near periapsis. As a practical matter this means that one cannot get a highly accurate result 

Question: Verify the following claims with "True" or "False": The epoch of a planet was on 31 December 2016.It has an orbital period of 135589000.0 and its periapsis is 279142000000.
Answer: True