Where is it now
- Distance from Sun
- 0.722 AU
- True anomaly
- 336.73°
- Distance from Earth
- 1.358 AU
- As of
- 19 October 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
- 15h 44m 55s
- Declination
- -19° 49′ 34″
- Constellation
- Libra
- Distance from Earth
- 1.35 AU
- Elongation from the Sun
- 31.33° — 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
- 0.858 AU
- Eccentricity
- 0.1689
- Inclination
- 0.06°
- Orbital period
- 290.3 days
- Perihelion
- 0.713 AU
- Aphelion
- 1.003 AU
- Longitude of ascending node
- 92.56°
- Argument of periapsis
- 213.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.1 LD
- 0.0002 AU
- Tisserand (Jupiter)
- 6.865
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 51
- Data arc
- 3 days
- First observed
- 16 February 2020
- Last observed
- 19 February 2020
- Residual RMS
- 0.44 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 30.4
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 72 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-20 13:41 UTC close approach of 2020 DW. Catalogue miss distance 99.5 LD · 3.82 × 10⁷ km. The curve is the geocentric path from 2027-09-17 to 2027-09-23, 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 |
|---|---|---|---|---|
| 2027-09-20 13:41:00 | Earth | 0.2556 AU | 99.5 LD | 6.6 km/s |
| 2028-02-25 18:05:00 | Earth | 0.2191 AU | 85.3 LD | 10.8 km/s |
| 2031-06-14 10:17:00 | Venus | 0.1464 AU | 57.0 LD | 2.8 km/s |
| 2031-08-23 07:51:00 | Earth | 0.2908 AU | 113.2 LD | 8.3 km/s |
| 2031-09-02 02:37:00 | Venus | 0.0671 AU | 26.1 LD | 6.6 km/s |
| 2032-02-20 17:09:00 | Earth | 0.3822 AU | 148.7 LD | 16.1 km/s |
| 2035-08-01 17:22:00 | Earth | 0.302 AU | 117.5 LD | 8.8 km/s |
| 2039-01-02 21:32:00 | Earth | 0.4597 AU | 178.9 LD | 18.6 km/s |
| 2039-07-11 13:51:00 | Earth | 0.2989 AU | 116.3 LD | 8.6 km/s |
| 2042-12-28 13:19:00 | Earth | 0.3166 AU | 123.2 LD | 14 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