Title: 2006 QQ23
Content:   is classified as an Aten asteroid, which means that it is a near-Earth asteroid that crosses Earth's orbit at two points and has an orbital period of less than a year. Because it will come within 0.05 au of the Earth (MOID) and has an absolute magnitude (H) brighter than 22, is labelled as a potentially hazardous object. With a 12 year observation arc it has a well determined orbit and is not a threat for the foreseeable future. It orbits the Sun at a distance of 0.57–1.03 au in less than 9 months (263 days; semi-major axis of 0.80 au). Its orbit has an eccentricity of 0.28 and an inclination of 3.4° with respect to the ecliptic. The body's observation arc begins with its first observation at the Siding Spring Observatory on 21 August 2006.
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: (391211) 2006 HZ51
Content:  has a minimum orbital intersection distance (MOID) with Earth of 0.035385 AU, which translates into 13.8 lunar distances. This makes it a potentially hazardous asteroid, a body with a threatening close approach to the Earth, due to its low MOID and large size (absolute magnitude of 18.5). Such asteroids are defined to have an absolute magnitude of 22 or brighter – which generically corresponds to a diameter of approximately 140 meters – and a MOID that is smaller than 0.05 AU or 19.5 LD. Based on a short observation arc of only 1.1 days, it was originally thought to have a 1 in 6 million chance of hitting Earth on 21 June 2008. Further refinement of the orbit quickly eliminated the risk. The preliminary 2-day orbit solution on 28 April 2006 was at first thought to have a period of 7 years and a perihelion of approximately 1.1 AU (MPEC 2006-H58).
Title: 4672 Takuboku
Content:  On 13 June 2005, Takuboku occulted 9.3 magnitude star TYC 0312-00789-1, causing a predicted magnitude drop 6.8 during 4.3 seconds. The occultation was visible over the southern island of New Zealand only. Measurement of the asteroid's occultation dimensions 35.0&thinsp;×35.0 for its major and minor best-fit ellipse (the fit's quality code is 1).
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 JY26
Content:  Recent calculations indicate that it follows a horseshoe orbit with respect to the Earth. It had a close encounter with the Earth on 10 May 2006, at 0.0029 AU. Its orbital evolution is very chaotic and its orbit is difficult to predict beyond a few hundred years. Its orbit matches the expected properties of that of an object in the Arjuna-class.
Title: HD 131664
Content:  of the Sun's luminosity from its photosphere at an effective temperature of 5,901 K. The discovery of a planet in orbit around HD 131664 was announced on October 26, 2008 and designated HD 131664 b. The object was detected from Doppler measurements of the host star between 2004 and 2008. This planet or brown dwarf has mass of at least 18.15 times that of Jupiter and orbits in a long-period, eccentric orbit that completely overlaps the star's habitable zone. This period (1,951 days or 5.34 years) is among the dozen longest exoplanet periods known, as of 2009. Follow-up studies with the Hipparcos satellite further constrained the predicted mass of the companion, providing a best estimate of 23 Jupiter mass.
Title: HD 20367
Content:  In June 2002, an announcement was made that a Jupiter-mass or larger extrasolar planet had been found orbiting the star, with a period of 469.5 days and an eccentricity of 0.32. The eccentric nature of this planet's orbit meant that it spends part of each circuit around the star outside the habitable zone. However, subsequent observations put the existence of this planet in doubt.
Title: (394130) 2006 HY51
Content:  orbits the Sun at a distance of 0.1–5.1 AU once every 4 years and 2 months (1,527 days). Its orbit has an eccentricity of 0.97 and an inclination of 33° with respect to the ecliptic. It is the asteroid with the third-smallest known perihelion of any known object orbiting the Sun. Its extreme orbital eccentricity brings it within 0.081 AU of the Sun (26% of Mercury's perihelion) and as far as 5.118 AU from the Sun (making it a Jupiter-grazer). It has a minimum orbit intersection distance with Earth of 0.1064 AU, equivalent to 41.5 lunar distances. The small bodies with even more eccentric orbits are likely to suffer a rotational breakup by the age comparable to that of the Solar System, although 2006 HY51 itself is not expected to break.
Title: 2006 QQ23
Content:  On 10 August 2019 at 7:23 am UTC, safely passed 0.04977 au from Earth; travelling at around 4.67 km/s The asteroid was recovered on 14 July 2019, which extended the observation arc from 8 years to 12 years, and therefore it had a very small uncertainty in the 2019 approach. The uncertainty region in the close approach was ±60 km.

Question: Verify the following claims with "True" or "False": The orbital period of 3425 Hurukawa is 135589000.0 and it epoch date is 2006.12.31.
Answer: False