Title: 2006 RH120
Content:  Analysis has shown that solar-radiation pressure is perturbing its motion perceptibly. However, Paul Chodas in JPL's Solar System Dynamics Group suspects that the perturbations are consistent with expectations for a rocky object but not with old flight hardware. One hypothesis is that the object is a piece of lunar rock ejected by an impact. On 18 February 2008, the object was given a minor planet designation. The object made four Earth orbits of about three months each before being ejected after the June 2007 perigee. At that perigee, it dipped inside the Moon's orbit to a distance of 276845 km. became an Apollo-class asteroid in June 2007.
Title: 2006 LM1
Content:   is a trans-Neptunian object and retrograde damocloid on a highly eccentric, cometary-like orbit. It was first observed on 3 June 2006 by the Mount Lemmon Survey at the Mount Lemmon Observatory in Arizona, United States. The orbit of is highly uncertain as its observation arc is only spans 2 days. measures approximately 5 km in diameter, assuming a low albedo of 0.09.
Title: Claimed moons of Earth
Content:  On 14 September 2006, an object estimated at 5 meters in diameter was discovered in near-polar orbit around Earth. Originally thought to be a third-stage Saturn S-IVB booster from Apollo 12, it was later determined to be an asteroid and designated as. The asteroid re-entered solar orbit after 13 months and is expected to return to Earth orbit after 21 years.
Title: 2006 RH120
Content:  On 14 June 2007, made its fourth and last perigee of the most recent Earth encounter. It was 0.7 lunar distances at closest, with an apparent magnitude of 18.5–19.0. Astronomers at JPL Goldstone in California made radar astrometry measurements on 12, 14 and 17 June 2007.
Title: 2006 HH123
Content:  , also written as 2006 HH123, was a misidentified nonexistent object that had a short 1 day observation arc. It was formerly thought to be a lost object with an assumed eccentricity of 0.46. If it had been a scattered-disc object it would have had an absolute magnitude of 5.2, and been a possible dwarf planet. The preliminary orbital elements (as displayed in the infobox to the right) were calculated using only three observations over a period of one day; hence its orbit was very poorly known and it quickly became lost. Of the three discovery images, the first one is an unidentified object, the second one was identified as the main-belt asteroid, and the third image shows nothing at the measured position. The three observations of were deleted on 6 November 2014, and the provisional designation  is no longer listed in the Minor Planet Center database.
Title: 2006 RH120
Content:  was discovered on 14 September 2006 by Eric Christensen with the 27 in Schmidt camera of the Catalina Sky Survey in Arizona. "6R10DB9" was the Catalina Sky Survey's own discovery designation for this object, which usually would only be used on the MPC's NEO Confirmation Page (NEOCP) until an IAU designation was applied, if the object was classified as a minor object. It was added on 14 September to the NEOCP and subsequently removed with the explanation that it "was not a minor planet". Preliminary orbital calculations indicated it was captured by Earth's gravity from solar orbit of a period of about 11 months, which is similar to that of many spent rocket boosters dating to the Apollo program of the 1960s and early 1970s. 6R10DB was assigned the designation on 18 February 2008.
Title: 2004 HR56
Content:  and was visible between 25 April 25 to 10 May 2005. This find was documented as part of the FMO Project and was reported by six different observatories. Reports indicate that the object is about 74 meters wide and has an absolute magnitude of 23.28. The object could also be classified as a meteoroid, although the most common definition uses a diameter of 10 m as the demarcation. It orbits the Sun at a distance of 0.9–2.2 AU once every 23 months (708 days). Its orbit has an eccentricity of 0.44 and an inclination of 6° with respect to the ecliptic.
Title: 2007 VE191
Content:  listed at NEODyS with odds of 1 in 3 million for 27 November 2015 during the approach window. was discovered on 15 November 2007 by the Mount Lemmon Survey at an apparent magnitude of 20 using a 1.5 m reflecting telescope. On 28 November 2007, it passed 0.0128 AU from Earth. has an observation arc of 13 days with an uncertainty parameter of 7, which means its orbit is poorly constrained. was last observed on 28 November 2007. By 1 December 2007, the asteroid had faded to below magnitude 25. With an absolute magnitude of 23.6, is about 50–110 meters in diameter.
Title: 2006 RH120
Content:  is now in solar orbit as an Amor-class asteroid with an orbit completely outside of Earth's orbit. As of 2017, this object was 2 AU from Earth on the other side of the Sun. Systematic residuals in the positions of the object probably indicate that the model used to determine solar radiation pressure may be too simple to adequately describe its motion over a long period of time. The next near-Earth encounter is in August 2028 when the object will pass Earth at a relatively low speed of 136 m/s. For comparison, on 13 April 2029, asteroid 99942 Apophis will pass Earth at a relative speed of 7.4 km/s. is listed as part of the Near-Earth Object Human Space Flight Accessible Targets Study (NHATS).
Title: (391211) 2006 HZ51
Content:   is a bright, sub-kilometer asteroid on an eccentric orbit, classified as a near-Earth object and a potentially hazardous asteroid of the Amor group. It was discovered on 27 April 2006, by astronomers of the Catalina Sky Survey conducted at Mount Lemmon Observatory, Arizona, United States. During preliminary observations, it was thought to have a small chance of impacting Earth in 2008. The asteroid measures approximately half a kilometer in diameter and has an exceptionally high albedo.

Question: Verify the following claims with "True" or "False": Well it has an epoch date of December 31st 2006 and a mass of 5.7 kilograms.
Answer: True