2018 LV2 is an asteroid in the Aten orbit class. Its orbit takes it from 0.7 AU to 1.29 AU from the Sun; one orbit takes 360.8 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.096 AU
- True anomaly
- 234.04°
- Distance from Earth
- 0.51 AU
- As of
- 2 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
- 20h 41m 37s
- Declination
- -17° 47′ 28″
- Constellation
- Capricornus
- Distance from Earth
- 0.51 AU
- Elongation from the Sun
- 87° — well clear of the Sun
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
- 0.992 AU
- Eccentricity
- 0.2992
- Inclination
- 2.98°
- Orbital period
- 360.8 days
- Perihelion
- 0.695 AU
- Aphelion
- 1.289 AU
- Longitude of ascending node
- 197.38°
- Argument of periapsis
- 301.16°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.5 LD
- 0.0115 AU
- Tisserand (Jupiter)
- 6.078
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 44
- Data arc
- 14 days
- First observed
- 7 June 2018
- Last observed
- 21 June 2018
- Residual RMS
- 0.51 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 25.3
Discovery & classification
Close approaches 55 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-01-30 04:21 UTC close approach of 2018 LV2. Catalogue miss distance 113.2 LD · 4.35 × 10⁷ km. The curve is the geocentric path from 2027-01-27 to 2027-02-02, 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 |
|---|---|---|---|---|
| 2027-01-30 04:21:00 | Earth | 0.2909 AU | 113.2 LD | 10.4 km/s |
| 2027-08-28 03:43:00 | Earth | 0.269 AU | 104.7 LD | 7.3 km/s |
| 2028-01-18 19:18:00 | Earth | 0.2822 AU | 109.8 LD | 9.9 km/s |
| 2028-09-06 11:58:00 | Earth | 0.2517 AU | 98.0 LD | 7.1 km/s |
| 2029-01-05 16:13:00 | Earth | 0.2668 AU | 103.8 LD | 9.1 km/s |
| 2029-09-17 19:11:00 | Earth | 0.2247 AU | 87.5 LD | 6.6 km/s |
| 2029-12-22 21:27:00 | Earth | 0.2427 AU | 94.5 LD | 7.8 km/s |
| 2029-12-29 08:37:00 | Venus | 0.0595 AU | 23.1 LD | 8.3 km/s |
| 2030-10-01 21:33:00 | Earth | 0.1826 AU | 71.1 LD | 6 km/s |
| 2031-10-19 01:21:00 | Earth | 0.1224 AU | 47.6 LD | 5.6 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