2015 VW168
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| Orbital characteristics[1] | |
|---|---|
| Epoch May 5, 2025 | |
| Uncertainty parameter Uncertainty Parameter U | |
| Observation arc | Observation arc length |
| Aphelion | 44.610 au (6,673.6 Gm) |
| Perihelion | 41.344 au (6,185.0 Gm) |
| 42.98 au (6,430 Gm) | |
| Eccentricity | 0.038 |
| 281.748 y | |
| 108.9 | |
| Inclination | 1.95 |
| 96.78 | |
| 210.43 | |
2015 VW168 is a trans-Neptunian object.[2]
Satellite
in 2019 the Hubble Space Telescope discovered a 64km[3] moon around 2015 VW168.[4][5]
References
- ↑ "(2015 VW168)". Small-Body Database. JPL. Retrieved 2025-06-02.
- ↑ "2015 VW168". ftp.lowell.edu. Retrieved 17 May 2025.
- ↑ Johnston, Wm. Robert (December 15, 2019). "2015 VW168". Johnson's Archive. Retrieved 2025-06-02.
- ↑ Porter, Simon B.; et al. (June 2024). "Detection of Close Kuiper Belt Binaries with HST WFC3". The Planetary Science Journal. 5 (6). id. 143. arXiv:2406.02808. Bibcode:2024PSJ.....5..143P. doi:10.3847/PSJ/ad3f19.
- ↑ Kuznetsov, E.; et al. (December 2021). "Dynamic evolution of pairs of trans-Neptunian objects: the case of binary and single objects in pair". Contributions of the Astronomical Observatory Skalnaté Pleso. 51 (3): 226–240. Bibcode:2021CoSka..51..226K. doi:10.31577/caosp.2021.51.3.226.
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