Where is it now
- Distance from Sun
- 1.197 AU
- True anomaly
- 168.11°
- Distance from Earth
- 0.405 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
- 20h 53m 26s
- Declination
- +11° 34′ 20″
- Constellation
- Delphinus
- Distance from Earth
- 0.41 AU
- Elongation from the Sun
- 109.86° — well clear of the Sun
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
- 0.851 AU
- Eccentricity
- 0.4291
- Inclination
- 20.82°
- Orbital period
- 286.8 days
- Perihelion
- 0.486 AU
- Aphelion
- 1.216 AU
- Longitude of ascending node
- 215.69°
- Argument of periapsis
- 344.89°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 57.5 LD
- 0.1478 AU
- Tisserand (Jupiter)
- 6.796
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 23
- Data arc
- 4.05 years
- First observed
- 19 October 2019
- Last observed
- 7 November 2023
- Residual RMS
- 0.68 ″
- Solution · Otto Matic
- 8 November 2023
Visual & observation
- Absolute magnitude (H)
- 23.24
Discovery & classification
Close approaches 209 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-11-11 11:09 UTC close approach of 2019 UN1. Catalogue miss distance 174.2 LD · 6.69 × 10⁷ km. The curve is the geocentric path from 2027-11-08 to 2027-11-14, 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 south 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 |
|---|---|---|---|---|
| 2027-11-11 11:09:00 | Earth | 0.4475 AU | 174.2 LD | 25.9 km/s |
| 2030-06-16 17:42:00 | Earth | 0.4744 AU | 184.6 LD | 17.8 km/s |
| 2030-10-22 00:20:00 | Earth | 0.2321 AU | 90.3 LD | 13 km/s |
| 2031-02-09 22:47:00 | Earth | 0.4889 AU | 190.3 LD | 15.1 km/s |
| 2033-09-17 05:55:00 | Earth | 0.4961 AU | 193.1 LD | 24.4 km/s |
| 2034-11-17 09:39:00 | Earth | 0.1604 AU | 62.4 LD | 15.2 km/s |
| 2037-09-19 06:43:00 | Earth | 0.286 AU | 111.3 LD | 13.6 km/s |
| 2038-04-04 23:45:00 | Merc | 0.0776 AU | 30.2 LD | 24.5 km/s |
| 2038-04-04 23:45:00 | Mercury | 0.0776 AU | 30.2 LD | 24.5 km/s |
| 2038-11-09 21:32:00 | Earth | 0.4826 AU | 187.8 LD | 27.1 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