 Zoozve photographed by theZwicky Transient Facility in November 2018 | |
| Discovery[1] | |
|---|---|
| Discovered by | LONEOS |
| Discovery site | Anderson Mesa Stn. |
| Discovery date | 11 November 2002 |
| Designations | |
| (524522) Zoozve | |
| 2002 VE68 | |
| Orbital characteristics[2] | |
| Epoch 5 September 2014 (JD 2456905.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 16.06yr (5,866 d) |
| Aphelion | 1.0206AU |
| Perihelion | 0.4268 AU |
| 0.7237 AU | |
| Eccentricity | 0.4103 |
| 225 days | |
| 251.64° | |
| 1° 36m 3.6s / day | |
| Inclination | 9.0060° |
| 231.58° | |
| 355.45° | |
| Earth MOID | 0.027 AU (10.44LD) |
| Physical characteristics | |
| 236 m (calculated)[3] | |
| 13.50±0.01 h[3][4] | |
| 0.20 (assumed)[3] | |
524522 Zoozve (/ˈzuːzveɪ/ ⓘ;provisional designation2002 VE68) is a sub-kilometer sizedasteroid and temporaryquasi-satellite ofVenus.[5] Discovered in 2002, it was the first such object to be discovered around a majorplanet in theSolar System. It has nearly the same orbital period around the Sun that Venus does. In a frame of reference rotating with Venus, it appears to travel around it during one Venerean year, but it orbits the Sun, not Venus.[6]
Zoozve was discovered on 11 November 2002 byBrian A. Skiff atLowell Observatory.[7][8] As of February 2013, it has been observed telescopically 457 times with a data-arc span of 2,947 days, and it was the target of Doppler observations on five occasions; therefore, itsorbit is very well determined. Its semi-major axis of 0.7237 AU is very similar to that of Venus, but its eccentricity is relatively large (0.4104), and its orbital inclination is also significant (9.0060°). The spectrum of Zoozve implies that it is anX-type asteroid and hence analbedo of about 0.25 should be assumed.[9] The body is calculated to measure 236 meters in diameter. Itsrotational period is 13.5 hours, and itslight curve has an amplitude of 0.9 mag, which hints at a very elongated body, perhaps acontact binary.[9]
The existence of retrograde satellites or quasi-satellites was first considered by J. Jackson in 1913[10] but none were discovered until almost 90 years later.[6] Zoozve was the first quasi-satellite to be discovered, in 2002, although it was not immediately recognized as such. Zoozve was identified as a quasi-satellite of Venus bySeppo Mikkola, Ramon Brasser,Paul A. Wiegert and Kimmo Innanen in 2004, two years after the actual discovery of the object.[5][6] From the perspective of a hypothetical observer in a frame of reference rotating with Venus, it appears to travel around the planet during one Venusian year. However, it does not orbit Venus, but instead orbits the Sun, like any otherasteroid. As a quasi-satellite, this minor body is trapped in a 1:1 mean-motion resonance with Venus. Besides being a Venusco-orbital, thisAten asteroid is also aMercury grazer and anEarth crosser. Zoozve exhibitsresonant (or near-resonant) behavior withMercury, Venus andEarth.[11][12] It seems to have been co-orbital with Venus for only the last 7,000 years, and is destined to be ejected from this orbital arrangement about 500 years from now.[6] During this time, its distance to Venus has been and will remain larger than about 0.2 astronomical units (30,000,000 km; 19,000,000 mi).
Zoozve is included in theMinor Planet Center list of Potentially Hazardous Asteroids (PHAs) because it comes relatively frequently to within 0.05 AU of Earth. Approaches as close as 0.04 AU occur with a periodicity of 8 years due to itsnear 8:13 resonance with Earth.[11] Zoozve was discovered during the close approaches of 11 November 2002. It approached Earth on 7 November 2010, again on 4 November 2018, and its next fly-by with Earth will happen on 2 November 2026 within 0.0402 AU (15.7 Lunar distances).[2]Numerical simulations indicate that an actualcollision with Earth during the next 10,000 years is not likely, although dangerously close approaches to about 0.002 AU are possible, a distance potentially within Earth'sHill sphere.[11]
Thisminor planet was numbered by theMinor Planet Center on 18 May 2019 (M.P.C. 114620).[13]
On 26 January 2024,Radiolab aired an episode about the asteroid, which co-hostLatif Nasser first noticed on his child's solar system poster, where it was referred to as "ZOOZVE", derived from the artist, Alex Foster, misreading his notes regarding the asteroid's provisional designation "2002VE".[8] This led Skiff to propose the name "Zoozve", on Nasser's behalf, to theInternational Astronomical Union's Working Group Small Bodies Nomenclature (WGSBN).[14] The name was approved and announced by the WGSBN on 5 February 2024.[15]
