Where is it now
- Distance from Sun
- 0.724 AU
- True anomaly
- 42.39°
- Distance from Earth
- 1.659 AU
- As of
- 23 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 10m 18s
- Declination
- -06° 36′ 25″
- Constellation
- Virgo
- Distance from Earth
- 1.67 AU
- Elongation from the Sun
- 12.59° — too close to the Sun to observe
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
- 0.965 AU
- Eccentricity
- 0.2947
- Inclination
- 4.72°
- Orbital period
- 346.4 days
- Perihelion
- 0.681 AU
- Aphelion
- 1.25 AU
- Longitude of ascending node
- 23.84°
- Argument of periapsis
- 113.43°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.2 LD
- 0.0004 AU
- Tisserand (Jupiter)
- 6.211
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 18
- Data arc
- 8 days
- First observed
- 6 October 2021
- Last observed
- 14 October 2021
- Residual RMS
- 0.56 ″
- Solution · Otto Matic
- 26 October 2021
Visual & observation
- Absolute magnitude (H)
- 28.14
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 99 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-06-23 06:07 UTC close approach of 2021 TH13. Catalogue miss distance 186.4 LD · 7.17 × 10⁷ km. The curve is the geocentric path from 2035-06-20 to 2035-06-26, 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 |
|---|---|---|---|---|
| 2035-06-23 06:07:00 | Earth | 0.479 AU | 186.4 LD | 22.7 km/s |
| 2036-04-15 11:52:00 | Venus | 0.0164 AU | 6.4 LD | 7.5 km/s |
| 2036-06-08 06:49:00 | Earth | 0.1784 AU | 69.4 LD | 13.5 km/s |
| 2037-06-05 20:39:00 | Earth | 0.1457 AU | 56.7 LD | 5.2 km/s |
| 2038-03-08 13:40:00 | Earth | 0.2932 AU | 114.1 LD | 10.1 km/s |
| 2038-08-08 08:54:00 | Earth | 0.2532 AU | 98.5 LD | 7.1 km/s |
| 2039-01-22 16:11:00 | Earth | 0.3053 AU | 118.8 LD | 10.5 km/s |
| 2039-09-28 01:09:00 | Earth | 0.1692 AU | 65.8 LD | 6 km/s |
| 2040-10-14 06:16:00 | Earth | 0.1167 AU | 45.4 LD | 12.1 km/s |
| 2041-10-01 17:00:00 | Earth | 0.4187 AU | 162.9 LD | 21.2 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