Where is it now
- Distance from Sun
- 0.65 AU
- True anomaly
- 79.6°
- Distance from Earth
- 0.397 AU
- As of
- 20 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
- 13h 51m 20s
- Declination
- +13° 11′ 44″
- Constellation
- Boötes
- Distance from Earth
- 0.4 AU
- Elongation from the Sun
- 23.94° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.882 AU
- Eccentricity
- 0.4508
- Inclination
- 18.32°
- Orbital period
- 302.8 days
- Perihelion
- 0.485 AU
- Aphelion
- 1.28 AU
- Longitude of ascending node
- 344.24°
- Argument of periapsis
- 328.66°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 32.6 LD
- 0.0837 AU
- Tisserand (Jupiter)
- 6.594
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 56
- Data arc
- 5.02 years
- First observed
- 25 February 2018
- Last observed
- 4 March 2023
- Residual RMS
- 0.38 ″
- Solution · Otto Matic
- 8 March 2023
Visual & observation
- Absolute magnitude (H)
- 23.28
Discovery & classification
Close approaches 215 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-10-25 19:15 UTC close approach of 2018 DA2. Catalogue miss distance 153.2 LD · 5.89 × 10⁷ km. The curve is the geocentric path from 2026-10-22 to 2026-10-28, 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 north 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 |
|---|---|---|---|---|
| 2026-10-25 19:15:00 | Earth | 0.3937 AU | 153.2 LD | 14.7 km/s |
| 2027-01-14 17:55:00 | Earth | 0.3618 AU | 140.8 LD | 11.9 km/s |
| 2028-03-14 10:08:00 | Earth | 0.1961 AU | 76.3 LD | 20.3 km/s |
| 2031-10-06 08:03:00 | Earth | 0.438 AU | 170.5 LD | 18.5 km/s |
| 2032-01-31 01:23:00 | Earth | 0.361 AU | 140.5 LD | 12.6 km/s |
| 2033-03-09 20:42:00 | Earth | 0.3375 AU | 131.4 LD | 24.9 km/s |
| 2036-08-31 08:14:00 | Merc | 0.0956 AU | 37.2 LD | 20.6 km/s |
| 2036-08-31 08:14:00 | Mercury | 0.0956 AU | 37.2 LD | 20.6 km/s |
| 2036-09-18 21:56:00 | Earth | 0.4741 AU | 184.5 LD | 21.3 km/s |
| 2037-02-13 03:54:00 | Earth | 0.3322 AU | 129.3 LD | 12.8 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