Title: HD 132563
Content:  Based upon radial velocity variations of HD 132563B, the presence of an ordinary giant planet has been inferred by S. Desidera et al. (2011). This object is orbiting the star with a period of 1,544 days, at a distance of about 2.6 AU, and with an orbital eccentricity of 0.22.
Title: HD 131496
Content:  A planet with a mass roughly 2.2 times that of Jupiter orbiting at a distance of 2.09 astronomical units (AU) once every 883 days was discovered in 2011. HD 131496 and its planet, HD 131496b, were chosen as part of the 2019 NameExoWorlds campaign organised by the International Astronomical Union, which assigned each country a star and planet to be named. HD 131496 was assigned to Andorra. The winning proposal for the name of the star was Arcalís, after a mountain peak in northern Andorra where the Sun shines through a gap twice a year at fixed dates, leading to its use as a primitive Solar calendar. The planet was named Madriu, after a glacial valley and river in southeastern Andorra that forms the major part of the Madriu-Perafita-Claror UNESCO world heritage site.
Title: HD 133131
Content:  In 2016 two planets planets orbiting HD 133131 A and one planet orbiting HD 133131 B were discovered utilizing the radial velocity method.
Title: HD 13931 b
Content:  HD 13931 b (also known as HIP 10626 b) is an extrasolar planet which orbits the G-type star HD 13931, located approximately 155 light years away in the constellation Andromeda. This planet takes 11.55 years to orbit the star at the average distance of 5.15 AU or 770 Gm. The planet's eccentricity (0.02) is about the same as Earth. The orbital distance for this planet ranges from 5.05 to 5.25 AU. This planet was discovered by using radial velocity method from spectrograph taken at Keck Observatory on November 13, 2009.
Title: HD 88133
Content:  In 2004 a planet was found to orbit the star utilizing a radial velocity method. In 2016-2017 the direct detection of the planetary thermal emission was claimed, but the detection was questioned in 2021.
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 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: 1319 Disa
Content:  Disa orbits the Sun in the outer main-belt at a distance of 2.4–3.6 AU once every 5 years and 2 months (1,884 days). Its orbit has an eccentricity of 0.21 and an inclination of 3° with respect to the ecliptic. It was first identified as at Heidelberg Observatory in 1908. The body's observation arc begins in 1929, when it was identified as at the discovering observatory, 6 years prior to its official discovery observation.
Title: HIP 13044
Content:  In 2010, it was announced that a giant planet in a 16.2-day orbit had been discovered by the radial velocity measurements. This would have had implications for planet formation in metal-poor systems and survival of planets being engulfed by expanded giant stars. Subsequent analysis of the data revealed problems with the detection: for example an erroneous barycentric correction had been applied (the same error had also led to claims of planets around HIP 11952 that were subsequently refuted). After applying the corrections, there is no evidence for a planet orbiting the star.
Title: (31345) 1998 PG
Content:  orbits the Sun at a distance of 1.2–2.8 AU once every 2 years and 10 months (1,046 days). Its orbit has an eccentricity of 0.39 and an inclination of 7° with respect to the ecliptic. A first precovery was taken at Palomar Observatory in 1978, extending the body's observation arc by 20 years prior to its official discovery observation at Anderson Mesa.

Question: Verify the following claims with "True" or "False": A planet (formerly"1928 PC") has an orbital period of 135589000.0 and the epoch is on 31 December 2016.
Answer: True