2019 EO is an asteroid in the Aten orbit class. Its orbit takes it from 0.46 AU to 1.52 AU from the Sun; one orbit takes 361.9 days. Orbit from the JPL solution of 27 February 2022.
Where is it now
- Distance from Sun
- 0.597 AU
- True anomaly
- 291.23°
- Distance from Earth
- 1.097 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
- 16h 49m 26s
- Declination
- -23° 14′ 58″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.08 AU
- Elongation from the Sun
- 32.56° — 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
- 0.994 AU
- Eccentricity
- 0.5325
- Inclination
- 9.35°
- Orbital period
- 361.9 days
- Perihelion
- 0.465 AU
- Aphelion
- 1.523 AU
- Longitude of ascending node
- 130.25°
- Argument of periapsis
- 255.54°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 17.7 LD
- 0.0456 AU
- Tisserand (Jupiter)
- 5.965
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 48
- Data arc
- 2.99 years
- First observed
- 2 March 2019
- Last observed
- 26 February 2022
- Residual RMS
- 0.38 ″
- Solution · Otto Matic
- 27 February 2022
Visual & observation
- Absolute magnitude (H)
- 23.18
Discovery & classification
Close approaches 199 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-12-19 17:42 UTC close approach of 2019 EO. Catalogue miss distance 164.5 LD · 6.32 × 10⁷ km. The curve is the geocentric path from 2026-12-16 to 2026-12-22, 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 |
|---|---|---|---|---|
| 2026-12-19 17:42:00 | Earth | 0.4227 AU | 164.5 LD | 14.1 km/s |
| 2027-03-05 15:25:00 | Earth | 0.3919 AU | 152.5 LD | 11.6 km/s |
| 2027-12-12 05:21:00 | Earth | 0.4482 AU | 174.4 LD | 16.1 km/s |
| 2028-03-09 13:40:00 | Earth | 0.4229 AU | 164.6 LD | 11.9 km/s |
| 2028-12-04 15:02:00 | Earth | 0.4692 AU | 182.6 LD | 17.7 km/s |
| 2029-03-14 06:47:00 | Earth | 0.4497 AU | 175.0 LD | 12.2 km/s |
| 2029-11-28 13:25:00 | Earth | 0.4866 AU | 189.4 LD | 19.2 km/s |
| 2030-03-18 15:25:00 | Earth | 0.4731 AU | 184.1 LD | 12.5 km/s |
| 2031-03-22 20:57:00 | Earth | 0.493 AU | 191.9 LD | 12.7 km/s |
| 2037-09-14 19:15:00 | Venus | 0.1404 AU | 54.6 LD | 25.3 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