Title: 316 Goberta
Content:  Goberta (minor planet designation: 316 Goberta) is a mid-sized Themistian asteroid that was discovered by French astronomer Auguste Charlois on 8 September 1891 in Nice. The light curve of 316 Goberta shows a periodicity of 8.605 ± 0.01 hours, during which time the brightness of the object varies by 0.20 ± 0.05 in magnitude.
Title: 3047 Goethe
Content:   Goethe is a non-family asteroid of the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.6–2.7 AU once every 4 years and 3 months (1,569 days; semi-major axis of 2.64 AU). Its orbit has a low eccentricity of 0.03 and a low inclination of 2° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Palomar in September 1960. In May 2156, it will pass at 0.0497 AU from the asteroid 29 Amphitrite at a relative velocity of 1.66 km/s.
Title: 1665 Gaby
Content:  Gaby orbits the Sun at a distance of 1.9–2.9 AU once every 3 years and 9 months (1,370 days). Its orbit has an eccentricity of 0.21 and an inclination of 11° with respect to the ecliptic. No precoveries were taken, and no prior identifications were made of Gaby. The body's observation arc begins 2 months after its official discovery observation at Heidelberg.
Title: 6489 Golevka
Content:  work by high-precision radar observations of Golevka. Between 1991 and 2003, the small force of the Yarkovsky effect caused a shift of 15 km from what would be expected based on only gravitational interactions. This helped evaluate the asteroid's bulk density (2.7 ± 0.5 g/cm3) and mass (2.10 kg). Golevka approaches Earth to 0.05 AU in 2046, 0.10 AU in 2069, and 0.11 AU in 2092. On the other hand, Golevka's collision probability with any planet is negligible for at least the next nine centuries. Its orbit is strikingly similar to that of 4179 Toutatis in eccentricity, semi-major axis, and inclination. However, Toutatis is better known due to a close approach to Earth in 2004.
Title: 1226 Golia
Content:  Golia orbits the Sun in the central main-belt at a distance of 2.3–2.9 AU once every 4 years and 2 months (1,516 days). Its orbit has an eccentricity of 0.11 and an inclination of 10° with respect to the ecliptic. The body's observation arc begins at Johannesburg one night after its official discovery observation, with no precoveries taken and no prior identifications made.
Title: 2010 GA6
Content:  is an Apollo asteroid. Apollo's cross the orbit of Earth and are the largest group of near-Earth objects with nearly 10 thousand known members. It orbits the Sun in the inner main-belt at a distance of 0.93–3.69 AU once every 3 years and 6 months (1,281 days; semi-major axis of 2.31 AU). Its orbit has a high eccentricity of 0.60 and an inclination of 10° with respect to the ecliptic. With an aphelion of 3.69 AU, it is also a Mars-crossing asteroid, as it crosses the orbit of the Red Planet at 1.666 AU.
Title: 3267 Glo
Content:  Glo is an eccentric member of the Phocaea family (701), that orbits the Sun in the inner asteroid belt at a distance of 1.6–3.0 AU once every 3 years and 7 months (1,299 days; semi-major axis of 2.33 AU). Its orbit has an eccentricity of 0.30 and an inclination of 24° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Anderson Mesa in January 1981.
Title: 2937 Gibbs
Content:  Gibbs is a Mars-crossing asteroid, as it crosses the orbit of Mars at 1.666 AU. It is also an eccentric member of the Phocaea family, a large asteroid family of stony asteroids in the inner main-belt. Gibbs orbits the Sun at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,290 days). Its orbit has an eccentricity of 0.30 and an inclination of 22° with respect to the ecliptic. The asteroid's observation arc begins with its official discovery observation at Anderson Mesa. No prior identifications were made and no precoveries taken.
Title: Gemini 3
Content: Mass: 3236.9 kg ; Perigee: 161.2 km ; Apogee: 224.2 km ; Inclination: 32.6 degrees ; Period: 88.3 minutes 
Title: Exploration of Io
Content:  For the next two and a half centuries, because of the satellite's small size and distance, Io remained a featureless, 5th-magnitude point of light in astronomers' telescopes. So, the determination of its orbital period, along with those of the other Galilean satellites, was an early focus for astronomers. By June 1611, Galileo himself had determined that Io's orbital period was 42.5 hours long, only 2.5 minutes longer than the modern estimate. Simon Marius' estimate was only one minute longer in the data published in Mundus Iovalis. The orbital periods generated for Io and the other Jovian satellites provided an additional validation for Kepler's Third Law of planetary motion. From these estimates 

Question: Verify the following claims with "True" or "False": The minor planet, 316 Goberta, has an apoapsis of 520906000.0 km and an average speed of 16.54 km/s.
Answer: False