2019 XS
Goldstone radar images of 2019 XS taken on 11 November 2021
Discovery [1][2]
Discovered byMLS
Discovery siteMt. Lemmon Obs.
Discovery date2 December 2019
Designations
2019 XS
C1HDFQ2 [3]
NEO · Apollo [4]
Orbital characteristics [4]
Epoch 21 January 2022 (JD 2459600.5)
Uncertainty parameter 0
Observation arc21.68 yr (7,919 days)
Earliest precovery date4 April 2000
Aphelion1.332 AU
Perihelion0.6766 AU
1.005 AU
Eccentricity0.3264
1.01 yr (367.74 days)
140.339°
0° 58m 44.218s / day
Inclination4.447°
49.483°
250.285°
Earth MOID0.004003 AU (598,800 km)
Physical characteristics
Mean diameter
~70 m [5]
2.35±0.01 h[6]
3.01±0.01 h[6]
23.96±0.33 [4]
23.87 [1]

    2019 XS is a small Apollo near-Earth asteroid discovered on 2 December 2019 by the Mount Lemmon Survey in Arizona, United States.[2] It passed 1.493 lunar distances (574,000 km; 357,000 mi) from Earth on 9 November 2021 at 03:48 UTC, after which observations were checked by the International Asteroid Warning Network for timing and astrometric accuracy.[7][8][9] During the close pass, the asteroid trailed across the far Southern Hemisphere to the Northern Hemisphere and reached a peak apparent magnitude of 13. A total of 957 observations were collected by Minor Planet Center as part of the International Asteroid Warning Network's campaign.[10]

    2019 XS is well-observed with a long observation arc of over 21 years, enough to distinguish subtle changes in its orbit over time due non-gravitational acceleration by the Yarkovsky effect.[4][10] Highly precise radar observations by NASA's Goldstone Solar System Radar on 11 November 2021 have significantly constrained the asteroid's orbit and 2021 close approach distance to within a few kilometres.[4] Radar imaging has shown that the asteroid is roughly 70 m (230 ft) in diameter, with a rotation period around 3 hours.[5]

    Continuous photometric observations by the Center for Solar System Studies in Landers, California show an irregular light curve for 2019 XS, signifying that the asteroid is in a tumbling rotation state.[6] The light curve of 2019 XS appears to display two overlapping periods of 2.35 and 3.01 hours, which could possibly be associated with the asteroid's rotation and precession.[6]

    Exploration

    2019 XS may be a potential target for the LICIACube mission after the completion of its primary mission.[11]

    See also

    • 2012 TC4, another near-Earth asteroid with a dedicated IAWN timing campaign

    References

    1. 1 2 "2019 XS". Minor Planet Center. International Astronomical Union. Retrieved 12 October 2021.
    2. 1 2 "MPEC 2019-X47 : 2019 XS". Minor Planet Electronic Circular. Minor Planet Center. 4 December 2019. Retrieved 12 October 2021.
    3. ↑ "2019 XS". NEO Exchange. Las Cumbres Observatory. 5 October 2021. Retrieved 12 October 2021.
    4. 1 2 3 4 5 "JPL Small-Body Database Browser: (2019 XS)" (2021-12-09 last obs.). Jet Propulsion Laboratory. Retrieved 7 January 2022.
    5. 1 2 Benner, Lance A. M. "Goldstone Radar Observations Planning: Orpheus, 2004 UE, 2019 XS, and 2010 VK139". Jet Propulsion Laboratory. California Institute of Technology. Retrieved 12 November 2021.
    6. 1 2 3 4 Warner, Brian D.; Stephens, Robert D. (April 2022). "Near-Earth Asteroid Lightcurve Analysis at the Center for Solar System Studies: 2021 October-December". The Minor Planet Bulletin. 49 (2): 83–89. Bibcode:2022MPBu...49...83W.
    7. ↑ "2019 XS: Timing Assessment". International Asteroid Warning Network. 3 October 2021. Retrieved 12 October 2021.
    8. ↑ "MPEC 2021-T79 : International Asteroid Warning Network (IAWN) Timing Campaign". Minor Planet Electronic Circular. Minor Planet Center. 5 October 2021. Retrieved 12 October 2021.
    9. ↑ "MPEC 2020-V63 : 2019 XS". Minor Planet Electronic Circular. Minor Planet Center. 10 November 2020. Retrieved 12 October 2021.
    10. 1 2 Farnocchia, Davide; Reddy, Vishnu; Bauer, James M.; Warner, Elizabeth M.; Micheli, Marco; Payne, Matthew J.; et al. (July 2022). "International Asteroid Warning Network Timing Campaign: 2019 XS". The Planetary Science Journal. 3 (7): 13. Bibcode:2022PSJ.....3..156F. doi:10.3847/PSJ/ac7224. hdl:10045/125567. 156.
    11. ↑ LICIACube [@LICIACube] (27 October 2022). "Michèle Lavagna: "Il lavoro di #LICIACube non finisce qui, abbiamo uno strumento prezioso e funzionante e ora stiamo decidendo verso quali corpi celesti orientarlo" https://t.co/9dxfUEW35n" [Michèle Lavagna: "The work of #LICIACube does not end here, we have a precious and functional tool and now we are deciding which celestial bodies to direct it towards"] (Tweet) (in Italian). Archived from the original on 14 November 2022. Retrieved 26 December 2022 – via Twitter.
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