2019 VT2 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.81 AU to 1.26 AU from the Sun; one orbit takes 384.7 days. Orbit from the JPL solution of 25 June 2022.
Where is it now
- Distance from Sun
- 1.213 AU
- True anomaly
- 150.05°
- Distance from Earth
- 1.574 AU
- As of
- 4 November 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 18h 09m 58s
- Declination
- -16° 20′ 54″
- Constellation
- Sagittarius
- Distance from Earth
- 1.57 AU
- Elongation from the Sun
- 50.41° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 1.035 AU
- Eccentricity
- 0.2149
- Inclination
- 9.26°
- Orbital period
- 384.7 days
- Perihelion
- 0.813 AU
- Aphelion
- 1.258 AU
- Longitude of ascending node
- 228.7°
- Argument of periapsis
- 293.1°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 20.2 LD
- 0.0518 AU
- Tisserand (Jupiter)
- 5.886
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 72
- Data arc
- 2.67 years
- First observed
- 22 October 2019
- Last observed
- 24 June 2022
- Residual RMS
- 0.46 ″
- Solution · Otto Matic
- 25 June 2022
Visual & observation
- Absolute magnitude (H)
- 24.37
Discovery & classification
Close approaches 108 on record
Top-down view of the ecliptic, Earth at the centre, for the 2038-11-22 05:35 UTC close approach of 2019 VT2. Catalogue miss distance 81.6 LD · 3.14 × 10⁷ km. The curve is the geocentric path from 2038-11-19 to 2038-11-25, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. At closest approach the object is south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2038-11-22 05:35:00 | Earth | 0.2097 AU | 81.6 LD | 13.1 km/s |
| 2039-11-16 14:56:00 | Earth | 0.1322 AU | 51.5 LD | 6 km/s |
| 2040-09-20 01:12:00 | Earth | 0.2895 AU | 112.7 LD | 6.5 km/s |
| 2041-04-11 22:29:00 | Earth | 0.1793 AU | 69.8 LD | 6.9 km/s |
| 2042-06-08 04:35:00 | Earth | 0.1279 AU | 49.8 LD | 10.3 km/s |
| 2043-06-27 10:03:00 | Earth | 0.4383 AU | 170.6 LD | 19.4 km/s |
| 2057-11-14 13:22:00 | Earth | 0.4009 AU | 156.0 LD | 18.8 km/s |
| 2058-11-26 07:42:00 | Earth | 0.0813 AU | 31.6 LD | 9.2 km/s |
| 2059-10-22 12:19:00 | Earth | 0.223 AU | 86.8 LD | 6.3 km/s |
| 2060-02-22 08:30:00 | Earth | 0.224 AU | 87.2 LD | 6.5 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB