2019 VT3 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.9 AU to 1.18 AU from the Sun; one orbit takes 387.3 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.153 AU
- True anomaly
- 149.69°
- Distance from Earth
- 1.848 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
- 16h 54m 12s
- Declination
- -26° 56′ 07″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.85 AU
- Elongation from the Sun
- 33.1° — 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
- 1.04 AU
- Eccentricity
- 0.1319
- Inclination
- 7.81°
- Orbital period
- 387.3 days
- Perihelion
- 0.903 AU
- Aphelion
- 1.177 AU
- Longitude of ascending node
- 40.64°
- Argument of periapsis
- 93.12°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 2.1 LD
- 0.0054 AU
- Tisserand (Jupiter)
- 5.882
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 19
- Data arc
- 3 days
- First observed
- 5 November 2019
- Last observed
- 8 November 2019
- Residual RMS
- 0.64 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 28.2
Discovery & classification
Close approaches 24 on record
Top-down view of the ecliptic, Earth at the centre, for the 2036-11-03 20:14 UTC close approach of 2019 VT3. Catalogue miss distance 100.2 LD · 3.85 × 10⁷ km. The curve is the geocentric path from 2036-10-31 to 2036-11-06, 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. 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 |
|---|---|---|---|---|
| 2036-11-03 20:14:00 | Earth | 0.2574 AU | 100.2 LD | 11.8 km/s |
| 2037-10-27 03:34:00 | Earth | 0.1192 AU | 46.4 LD | 4.2 km/s |
| 2038-06-11 16:18:00 | Earth | 0.184 AU | 71.6 LD | 3.8 km/s |
| 2039-05-08 19:57:00 | Earth | 0.1819 AU | 70.8 LD | 9.7 km/s |
| 2053-10-27 04:31:00 | Earth | 0.4407 AU | 171.5 LD | 17.1 km/s |
| 2054-11-10 15:47:00 | Earth | 0.0666 AU | 25.9 LD | 6.6 km/s |
| 2055-08-25 02:17:00 | Earth | 0.2145 AU | 83.5 LD | 4 km/s |
| 2056-04-28 23:45:00 | Earth | 0.01 AU | 3.9 LD | 5.2 km/s |
| 2056-04-30 01:04:00 | Moon | 0.0093 AU | 3.6 LD | 5.3 km/s |
| 2057-05-14 00:01:00 | Earth | 0.3011 AU | 117.2 LD | 12.9 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