2020 VT1

{{DISPLAYTITLE:{{mp|2020 VT|1}}}}

{{Use dmy dates|date=February 2021}}

{{Infobox planet

| minorplanet = yes

| name = {{mp|2020 VT|1}}

| background = #FFC2E0

| image =

| image_size =

| caption =

| discovery_ref =

| discoverer = Pan-STARRS1

| discovery_site = Haleakalā Obs.

| discovered = 10 November 2020

| mpc_name = {{mp|2020 VT|1}}

| alt_names =

| pronounced =

| named_after =

| mp_category = NEOAmor

| orbit_ref =

| epoch = 31 May 2020 (JD 2459000.5)

| uncertainty = 6{{·}}5

| observation_arc = 24 days

| aphelion = 1.7774 AU

| perihelion = 1.2687 AU

| semimajor = 1.5231 AU

| eccentricity = 0.1670

| period = 1.88 yr (687 d)

| mean_anomaly = 315.41°

| mean_motion = {{Deg2DMS|0.5244|sup=ms}} / day

| inclination = 18.717°

| asc_node = 50.169°

| arg_peri = 296.19°

| moid = {{convert|0.3504|AU|LD|sigfig=3|abbr=on|lk=out}}

| mean_diameter = {{val|89|ul=m}} {{small|(est. at 0.15)}}

| rotation =

| albedo =

| spectral_type =

| abs_magnitude = 22.921{{·}}23.0

}}

{{mp|2020 VT|1}} is a small asteroid, classified as a near-Earth object of the Amor group, that is a temporary horseshoe companion to Mars.

Discovery

{{mp|2020 VT|1}} was discovered on 10 November 2020, by J. Bulger, K. Chambers, T. Lowe, A. Schultz, and M. Willman observing

for the survey conducted by Pan-STARRS at Haleakalā Observatory, Hawaii. As of 20 January 2021, it has been observed 28 times with an observation arc of 24 days.

Orbit and orbital evolution

{{mp|2020 VT|1}} is currently an Amor asteroid, a subgroup of the near-Earth objects that approach the orbit of Earth from beyond, but do not cross it. It orbits the Sun at a distance of 1.3–1.8 AU once every 23 months (687 days; semi-major axis of 1.52 AU). Its orbit has a moderate eccentricity of 0.17 and an inclination of 19° with respect to the ecliptic. It is most notable for its horseshoe orbit, a complex co-orbital motion with Mars, as both bodies have similar semi-major axes. The object can also be classified as a Mars-crosser, intersecting the orbit of the Red Planet at 1.66 AU.

{{multiple image | align = left| direction = horizontal | width = 260

| header = Animation of {{mp|2020 VT|1}} from 1600 to 2500

| image1 = Animation of 2020 VT1 around Sun - Frame rotating with Mars.gif

| caption1 = Relative to Sun and Mars

| image2 = Animation of 2020 VT1 around Mars.gif

| caption2 = Around Mars

| image3 = Animation of 2020 VT1 around Sun.gif

| caption3 = Around Sun

| footer ={{legend2| Yellow|Sun}}{{·}}{{legend2| Lime|Mars}}{{·}}{{legend2|Magenta|{{mp|2020 VT|1}} }}

}}

{{clear}}

Mars trojan

{{L4}} (leading):

  • {{mpl|(121514) 1999 UJ|7}} †

{{L5}} (trailing):

{{Div col|colwidth=16em}}

  • 5261 Eureka (1990 MB) †
  • {{mpl|(101429) 1998 VF|31}} †
  • {{mpl|(311999) 2007 NS|2}} †
  • {{mpl|(385250) 2001 DH|47}}
  • {{mpl|2009 SE|}}
  • {{mpl|2011 SC|191}}
  • {{mpl|2011 SL|25}}
  • {{mpl|2011 SP|189}}
  • {{mpl|2011 UB|256}}
  • {{mpl|2011 UN|63}}
  • {{mpl|2016 CP|31}}
  • {{mpl|2018 EC|4}}
  • {{mpl|2018 FC|4}}

{{Div col end}}

References

{{reflist|30em|refs=

{{cite web

|type = 2020-11-14 last obs.

|title = JPL Small-Body Database Browser: (2020 VT1)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=54087655

|publisher = Jet Propulsion Laboratory

|accessdate = 7 February 2021}}

{{cite web

|title = MPEC 2020-V75 : 2020 VT1

|url = https://www.minorplanetcenter.net/mpec/K20/K20V75.html

|work = Minor Planet Electronic Circular

|publisher = Minor Planet Center

|date = 12 November 2020

|access-date= 7 February 2021}}

{{cite web

|title = 2020 VT1

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=2020+VT1

|accessdate = 7 February 2021}}

{{cite web

|title = Asteroid Size Estimator

|publisher = CNEOS NASA/JPL

|url = https://cneos.jpl.nasa.gov/tools/ast_size_est.html

|accessdate = 7 February 2021}}

{{Cite journal|title=Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space |first1=Carlos |last1=de la Fuente Marcos |last2=de la Fuente Marcos |first2=Raúl |date=March 2021|journal=Monthly Notices of the Royal Astronomical Society|volume=501|issue=4|pages=6007–6025|doi=10.1093/mnras/stab062 |doi-access=free |arxiv = 2101.02563| bibcode = 2021MNRAS.501.6007D |url=https://academic.oup.com/mnras/article-abstract/501/4/6007/6081058}}

}}

;Further reading

  • [http://adsabs.harvard.edu/abs/2000Sci...288.2190B Understanding the Distribution of Near-Earth Asteroids] Bottke, W. F., Jedicke, R., Morbidelli, A., Petit, J.-M., Gladman, B. 2000, Science, Vol. 288, Issue 5474, pp. 2190–2194.
  • [http://adsabs.harvard.edu/abs/2000Icar..144....1C A Numerical Survey of Transient Co-orbitals of the Terrestrial Planets] Christou, A. A. 2000, Icarus, Vol. 144, Issue 1, pp. 1–20.
  • [http://adsabs.harvard.edu/abs/2002Icar..156..399B Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects] Bottke, W. F., Morbidelli, A., Jedicke, R., Petit, J.-M., Levison, H. F., Michel, P., Metcalfe, T. S. 2002, Icarus, Vol. 156, Issue 2, pp. 399–433.
  • [http://adsabs.harvard.edu/abs/2004Icar..171..102B Transient co-orbital asteroids] Brasser, R., Innanen, K. A., Connors, M., Veillet, C., Wiegert, P., Mikkola, S., Chodas, P. W. 2004, Icarus, Vol. 171, Issue 1, pp. 102–109.