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: 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:  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: 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: 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: 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: 2019 UN13
Content:  The close approach to Earth lifted the asteroid's aphelion point (furthest distance from the Sun) from 1.33 AU (inside the orbit of Mars) to 2.06 AU (near the edge of the inner asteroid belt). The approach changed the orbit from an Aten asteroid with a semi-major axis less than 1 AU to an Apollo asteroid with a semi-major axis greater than that of the Earth (&gt; 1 AU). With the new orbit, will come to perihelion 0.83 AU from the Sun on 15 December 2019. Without perturbations, the previous orbit would have come to perihelion in January 2020.
Title: Prognoz 9
Content: Mass: 1060 kg ; Periapsis: 380 km ; Apoapsis: 720000 km ; Period: 38448.0 min (26.7 days) ; Inclination: 65.5°.  The spacecraft with highly eccentric orbit was spin stabilized with a period of 113 s. The spin axis pointed towards the Sun, and was repointed every few days.
Title: ODERACS 2E
Content: COSPAR ID: 1995-004G ; SATCAT number: 23475 ; Mass: 5 kg ; Perigee: 314 km ; Apogee: 336 km ; Orbital period: 91 minutes ; Orbital inclination: 51.6° ; Eccentricity: 0.00164 ; Decay Date: February 27, 1995 
Title: (190166) 2005 UP156
Content:  This near-Earth object has an Earth minimum orbital intersection distance of 0.1316 AU which corresponds to 51.3 lunar distances. On 10 July 2017, it approached Earth to a distance of 0.133 AU and will make its next close approach at 0.128 AU in July 2057.

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