Title: 2011 CQ1
Content:   is a meteoroid discovered on 4 February 2011 by Richard A. Kowalski, at the Catalina Sky Survey. On the same day the meteoroid passed within 0.85 Earth radii (5480 km) of Earth's surface, and was perturbed from the Apollo class to the Aten class of near-Earth objects. With a relative velocity of only 9.7 km/s, had the asteroid passed less than 0.5 Earth radii from Earth's surface, it would have fallen as a brilliant fireball. The meteoroid is between 80 cm and 2.6 m wide. The meteoroid was removed from the Sentry Risk Table on 5 February 2011. It was not until 2020 QG on 16 August 2020 that a non-impacting closer approach to Earth was observed.
Title: 2011 EO40
Content:  was discovered by Richard A. Kowalski on 10 March 2011 while observing for the Mount Lemmon Survey. Its orbit is typical of Apollo asteroids and is characterized by significant eccentricity (0.54), low inclination (3.36º), and a semi-major axis of 1.65 AU. Upon discovery, it was classified as an Earth crosser, a near-Earth asteroid (NEA) and a potentially hazardous asteroid (PHA) by the Minor Planet Center. It was listed on the Sentry Risk Table for less than one day. Its orbit is in need of additional observations to determine if it is part of an asteroid family; as of October 2015 the orbit is determined using just twenty observations spanning an observation arc of 34 days. has an absolute magnitude of 21.5, which gives a characteristic diameter of about 200 m.
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: C/2011 L4
Content:  distance of 1.09 AU. It came to perihelion (closest approach to the Sun) on 10 March 2013. Original estimates predicted that C/2011 L4 would brighten to roughly apparent magnitude 0 (roughly the brightness of Alpha Centauri A or Vega). An estimate in October 2012 predicted that it might brighten to magnitude −4 (roughly equivalent to Venus). In January 2013 there was a noticeable brightening slowdown that suggested that it may only brighten to magnitude +1. During February the brightness curve showed a further slowdown suggesting a perihelion magnitude of around +2. However, a study using the secular light curve indicates that C/2011 L4 had a 
Title: C/2011 J2 (LINEAR)
Content:  C/2011 J2 (LINEAR) is an Oort cloud comet discovered on 4 May 2011 by LINEAR at an apparent magnitude of 19.7 using a 1 m Reflecting telescope. As of September 2014 the comet is around apparent magnitude 17. C/2011 J2 came to perihelion (closest approach to the Sun) on 25 December 2013 at a distance of 3.4 AU from the Sun. On 27 August 2014 an 18th magnitude fragment CK11J02b was detected. Preliminary estimates are that a fragmentation event occurred around 14 July 2014 plus/minus ten days. In mid-July 2014 the comet was 3.9 AU from the Sun. Fragment C was detected in October 2014 by Ernesto Guido, Nick Howes, and Martino Nicolini. C/2011 J2 is dynamically new. It came from the Oort cloud with a loosely bound chaotic orbit that was easily perturbed by galactic tides and passing stars. Before entering the planetary region (epoch 1950), C/2011 J2 had an orbital period of several million years. After leaving the planetary region (epoch 2050), it will be on an ejection trajectory.
Title: (24952) 1997 QJ4
Content:  , also written as 1997 QJ4, is a plutino and as such, it is trapped in a 2:3 mean-motion resonance with Neptune. It was discovered on 28 August, 1997, by Jane X. Luu, Chad Trujillo, David C. Jewitt and K. Berney. This object has a perihelion (closest approach to the Sun) at 30.463 AU and an aphelion (farthest approach from the Sun) at 48.038 AU, so it moves in a relatively eccentric orbit (0.224). It has an estimated diameter of 139 km; therefore, it is unlikely to be classified as a dwarf planet.
Title: 2015 KQ174
Content:  orbits the Sun at a distance of 49.3–61.5 AU once every 412 years and 4 months (150,600 days; semi-major axis of 55.4 AU). Its orbit has an eccentricity of 0.11 and an inclination of 24° with respect to the ecliptic. The object belongs to the same group as ("Buffy"),,  and  (also see diagram). With an orbital period of 412 years, it seems to be a resonant trans-Neptunian objects in a 2:5 resonance with Neptune, as several other objects, but with a lower eccentricity (0.11 instead of more than 0.60) and higher perihelia (at 49.3 AU rather than 31–41 AU). Considered both a scattered and detached object,  is particularly unusual as it has an unusually circular orbit for a scattered-disc object (SDO). Although 
Title: C/2001 Q4 (NEAT)
Content:  C/2001 Q4 (NEAT) is a comet with an unusual, almost perpendicular retrograde orbit which brings it into the inner Solar System by a deeply southward path. It initially emerged from its remote home spending most of its time near the south celestial pole. This comet was discovered on August 24, 2001 by the Near-Earth Asteroid Tracking program (NEAT). In 2004, residents of the southern hemisphere had the opportunity to watch the comet gradually brighten as it raced toward perihelion. On May 6, 2004 the comet approached within 0.32 AU of the Earth. Beginning in early May, the comet started racing north and burst into view in the northern hemisphere when it had reached almost maximum brightness. With a near perihelion orbital eccentricity of 1.00069 (epoch 2004-May-18) that keeps a barycentric epoch 2014-Jan-01 eccentricity of 1.00067, this hyperbolic comet is going to be ejected from the Solar System.
Title: 471143 Dziewanna
Content:  The minor planet orbits the Sun at a distance of 32.6–108.3 AU once every 591 years and 4 months (215,992 days). Its orbit has an eccentricity of 0.54 and an inclination of 29° with respect to the ecliptic. It is currently 39.1 AU from the Sun and will reach perihelion in 2038. A ten-million-year integration of the orbit shows that this object is in a 2:7 resonance with Neptune. A first precovery was taken by the Near-Earth Asteroid Tracking at Palomar Observatory in 2002, extending the minor planet's observation arc by 8 years prior to its discovery observation. Since then it has been observed 143 times over 6 oppositions and has an orbit quality of 1.
Title: (471325) 2011 KT19
Content:  was discovered by the Mount Lemmon Survey on 31 May 2011. Its rediscovery was announced in August 2016 by a team of astronomers using the Pan-STARRS telescope. It was soon linked with a supposed prograde centaur (inclination = 38° and semi-major axis = 28 AU) that had been lost due to a short observation arc. is in a 7:9 resonance with Neptune. Currently it is the only object with a nearly polar orbit that is in resonance with a planet. Notably, it is part of a group of objects that orbit the Sun in a highly inclined orbit; the reasons for this unusual orbit are unknown as of August 2016. The orbital characteristics of 

Question: Verify the following claims with "True" or "False": The epoch of 2011 CQ1 was on the 31st of July 2016 and its periapsis is 445895000000.0.
Answer: False