Title: 1097 Vicia
Content:  Vicia was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany on 11 August 1928. On 15 and 22 August, the asteroid was independently discovered by Soviet astronomer Pelageya Shajn at Simeiz Observatory on the Crimean peninsula, and by English astronomer Harry Edwin Wood at the Johannesburg Observatory in South Africa, respectively. However, the Minor Planet Center only recognizes the first discoverer. The asteroid was first identified as at Heidelberg in May 1907. The body's observation arc begins at Heidelberg in August 1928, six nights after its official discovery observation.
Title: 1097 Vicia
Content:  In November 2010, a rotational lightcurve of Vicia was obtained from photometric observations by Gordon Gartrelle at the University of North Dakota (730) and at the Badlands Observatory in North Dakota, United States. Analysis of the fragmentary lightcurve gave a rotation period of 26.5 hours with a brightness variation of 0.08 magnitude, indicative for a spherical rather than irregular and elongated shape (U=1). As of 2017, however, no other lightcurve has been obtained and Vicias rotation period has not yet been secured.
Title: 1097 Vicia
Content:  Vicia spectral type has not been determined. Asteroids in the central main belt with a semi-major axis between 2.6 and 2.7 AU, are located in a transitional region where both stony and carbonaceous asteroids are frequent and generic assumptions are difficult.
Title: 1097 Vicia
Content:  This minor planet was named after the flowering plant Vicia, member of the Fabaceae (legume family). It is commonly known as vetches. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 103).
Title: 1030 Vitja
Content:  Vitja is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.5 AU once every 5 years and 6 months (2,014 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.12 and an inclination of 15° with respect to the ecliptic. The asteroid's first recorded observation was made a week after its official discovery at Heidelberg Observatory in June 1924, while its observation arc begins more than seven years later at Lowell Observatory in October 1931.
Title: 2007 BP102
Content:   is a high inclination centaur and damocloid from the outer regions of the Solar System, approximately 34 kilometers in diameter. It was first observed by astronomers at the Mauna Kea Observatories on 24 January 2007. With a Tisserand's parameter of 1.99, may be considered a member of the damocloids, a dynamical group of minor planets which have comet-like orbits without showing a cometary coma or tail. It orbits the Sun at a distance of 17.7–30.2 AU once every 117 years and 6 months (42,907 days). Its orbit has an eccentricity of 0.26 and an inclination of 65° with respect to the ecliptic. As of July 2017, it is one of 7 known objects with inclination (i) > 60° and perihelion (q) > 15 AU, along with the first discovered.
Title: 174567 Varda
Content:  Varda was discovered in March 2006, using imagery dated from 21 June 2003 by Jeffrey A. Larsen with the Spacewatch telescope as part of a United States Naval Academy Trident Scholar project. It orbits the Sun at a distance of 39.5–52.7 AU once every 313.1 years (over 114,000 days; semi-major axis of 46.1 AU). Its orbit has an eccentricity of 0.14 and an inclination of 21.5° with respect to the ecliptic. , Varda is 47.5 AU from the Sun. It will come to perihelion around November 2096. It has been observed 321 times over 23 oppositions, with precovery images back to 1980.
Title: 977 Philippa
Content:  Philippa is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the outer asteroid belt at a distance of 3.0–3.2 AU once every 5 years and 6 months (2,011 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.03 and an inclination of 15° with respect to the ecliptic. The asteroid was first observed as A914 YA (1914 YA) at Heidelberg Observatory in December 1912. The body's observation arc begins at Vienna Observatory on 1 May 1922, or one month after its official discovery observation at Algiers.
Title: 13474 V'yus
Content:  V'yus is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 1.9–3.4 AU once every 4 years and 3 months (1,551 days; semi-major axis of 2.62 AU). Its orbit has an eccentricity of 0.29 and an inclination of 8° with respect to the ecliptic. The body's observation arc begins with its first identification as at Goethe Link Observatory in September 1956, almost 17 years prior to its official discovery observation at Nauchnyj.
Title: 1309 Hyperborea
Content:  Hyperborea is a non-family asteroid of the main belt's background population. It orbits the Sun in the outermost asteroid belt at a distance of 2.7–3.7 AU once every 5 years and 9 months (2,098 days; semi-major axis of 3.21 AU). Its orbit has an eccentricity of 0.15 and an inclination of 10° with respect to the ecliptic. The body's observation arc begins at Heidelberg Observatory with its first observations as in September 1919, or 12 years prior to its official discovery observation at Simeiz.

Question: Verify the following claims with "True" or "False": 1097 Vicia (formerly"1928 PC") has an orbital period of 135589000.0 and the epoch is on 31 December 2016.
Answer: True