Title: 1101 Clematis
Content:  Clematis is a member of the Alauda family (902), a large family of typically "bright" carbonaceous asteroids and named after its parent body, 702 Alauda. According to a different study, this object is also the namesake of the Clematis family, a small family of 5–16 asteroids hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination. It orbits the Sun in the outermost asteroid belt at a distance of 3.0–3.5 AU once every 5 years and 10 months (2,120 days; semi-major axis of 3.23 AU). Its orbit has an eccentricity of 0.08 and an inclination of 21° with respect to the ecliptic. The body's observation arc begins with its observation as at Goethe Link Observatory in October 1963, more than 35 years after its official discovery observation at Heidelberg.
Title: 1101 Clematis
Content:  1101 Clematis is an Alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter. It was discovered on 22 September 1928, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany, and assigned the provisional designation. It was named for the flowering plant Clematis. The presumably carbonaceous asteroid has a relatively long rotation period of 34.3 hours.
Title: 1101 Clematis
Content:  Clematis is an assumed carbonaceous C-type asteroids, while the overall spectral type for members of the Alauda family is that of a somewhat brighter B-type.
Title: 1101 Clematis
Content:  This minor planet was named after the flowering plant Clematis, a genus within the Ranunculaceae (buttercup or crowfoot family). The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H n.a.).
Title: 2010 BK118
Content:   (also written 2010 BK118) is a centaur roughly 20–60 km in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of ~400 AU. came to perihelion in April 2012 at a distance of 6.1 AU from the Sun (outside the orbit of Jupiter). It has a Jupiter-MOID of 1.1 AU. , it is 11 AU from the Sun. It will not be 50 AU from the Sun until 2043. After leaving the planetary region of the Solar System, will have a barycentric aphelion of 791 AU with an orbital period of 8000 years.
Title: 1140 Crimea
Content:  Crimea is a S-type asteroid in both the Tholen and SMASS taxonomic scheme. It orbits the Sun in the central main-belt at a distance of 2.5–3.1 AU once every 4 years and 7 months (1,685 days). Its orbit has an eccentricity of 0.11 and an inclination of 14° with respect to the ecliptic. First identified as at Simeiz in 1922, the body's observation arc begins at Uccle in 1935, or 16 years after its official discovery observation at Simeiz.
Title: Gemini 11
Content: Mass: 8374 lb Perigee: 156.4 nmi ; Apogee: 739.2 nmi ; Inclination: 28.85° ; Period: 101.52 min  Highest orbit (followed twice):
Title: Expedition 11
Content: Perigee: ~384 km ; Apogee: ~396 km ; Inclination: ~51.6° ; Orbital period: ~92 min 
Title: 3034 Climenhaga
Content:  Climenhaga is a member of the Flora family, one of the largest families of stony asteroids in the main belt. It orbits the Sun in the inner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,294 days). Its orbit has an eccentricity of 0.21 and an inclination of 5° with respect to the ecliptic. The asteroid's observation arc begins with its official discovery observation at Heidelberg, as no precoveries were taken, and no prior identifications were made.
Title: 1102 Pepita
Content:  Pepita 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 2.7–3.4 AU once every 5 years and 5 months (1,966 days; semi-major axis of 3.07 AU). Its orbit has an eccentricity of 0.11 and an inclination of 16° with respect to the ecliptic. In May 1899, the asteroid was first observed as at Harvard's Boyden Station in Arequipa, Peru (800). The body's observation arc begins with its official discovery observation at Barcelona.

Question: Verify the following claims with "True" or "False": 1101 Clematis has a periapsis of 445895000000.
Answer: True