2012 HZ84 orbits the Sun at a distance of 37.2–55.4 AU once every 315 years and 5 months (semi-major axis of 46.33 AU). Its orbit has an eccentricity of 0.20 and an inclination of 5.4° with respect to the ecliptic.[2]
As a cubewano, also known as classical Kuiper belt object,[4]2012 HZ84 is located in between the resonant plutino and twotino populations and has a low-eccentricity orbit. It belongs to the "stirred" hot population, but only just, since the rather arbitrary threshold to the cold population is typically defined for inclinations lower than 5°.
In the object classification of the Deep Ecliptic Survey, however, 2012 HZ84 has a secured SCATNEAR type, which is a combination of the SCAT and NEAR attributes. It means that the object does not cross the orbit of Neptune but has a higher inclination and eccentricity (SCAT) than the survey's CLASSICAL type objects, and it currently interacts with the dominant ice giant Neptune (NEAR), contrary to the much less gravitationally affected objects of the EXTD type.[3]
Trajectory of New Horizons and other nearby Kuiper belt objects
When the New Horizons spacecraft imaged 2012 HZ84 in 2017, it was the farthest from Earth ever captured by a spacecraft. The image was taken by the spacecraft's Long Range Reconnaissance Imager (LORRI) on 5 December 2017 at more than 6.12 billion kilometers (40.9 AU) away from Earth. This record was previously held by the Voyager 1 spacecraft which took the iconic Pale Blue Dot image at 6.06 billion kilometers from Earth in February 1990.[5]
In December 2017, New Horizons also imaged the trans-Neptunian object 2012 HE85, which was first observed by the same team of astronomers the night after they discovered 2012 HZ84.[5] Both objects held this record for little more than one year, until it was superseded on New Year's Eve 2018/19, when New Horizons made its close flyby of 486958 Arrokoth at a new record distance of 6.4 billion kilometers from Earth.[7]
According to Johnston's Archive, the object measures 74 kilometers in diameter based on an assumed albedo of 0.09 and an absolute magnitude of 8.9.[2][4] As of 2019, no rotational lightcurve of 2012 HZ84 has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[2]
