Where is it now
- Distance from Sun
- 0.6 AU
- True anomaly
- 67.07°
- Distance from Earth
- 1.578 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
- 14h 07m 38s
- Declination
- -10° 39′ 57″
- Constellation
- Virgo
- Distance from Earth
- 1.58 AU
- Elongation from the Sun
- 6.96° — 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
- 0.843 AU
- Eccentricity
- 0.4155
- Inclination
- 10.54°
- Orbital period
- 282.7 days
- Perihelion
- 0.493 AU
- Aphelion
- 1.193 AU
- Longitude of ascending node
- 193.11°
- Argument of periapsis
- 323.75°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 8.2 LD
- 0.021 AU
- Tisserand (Jupiter)
- 6.892
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 16
- Data arc
- 5 days
- First observed
- 5 October 2018
- Last observed
- 10 October 2018
- Residual RMS
- 0.29 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.5
Discovery & classification
Close approaches 48 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-08-28 09:50 UTC close approach of 2018 TD2. Catalogue miss distance 86.4 LD · 3.32 × 10⁷ km. The curve is the geocentric path from 2028-08-25 to 2028-08-31, 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 |
|---|---|---|---|---|
| 2028-08-28 09:50:00 | Earth | 0.2221 AU | 86.4 LD | 9.5 km/s |
| 2028-12-24 06:53:00 | Earth | 0.4163 AU | 162.0 LD | 11.6 km/s |
| 2031-06-17 16:12:00 | Venus | 0.1184 AU | 46.1 LD | 13.9 km/s |
| 2031-07-25 13:27:00 | Earth | 0.3212 AU | 125.0 LD | 19.3 km/s |
| 2032-10-03 01:19:00 | Earth | 0.3545 AU | 137.9 LD | 22.6 km/s |
| 2034-07-26 18:55:00 | Venus | 0.1236 AU | 48.1 LD | 19 km/s |
| 2036-09-09 20:51:00 | Venus | 0.1235 AU | 48.1 LD | 19.9 km/s |
| 2038-07-19 10:17:00 | Earth | 0.1954 AU | 76.1 LD | 13.1 km/s |
| 2039-02-06 13:14:00 | Earth | 0.4956 AU | 192.9 LD | 19.9 km/s |
| 2039-10-11 22:24:00 | Venus | 0.102 AU | 39.7 LD | 13.4 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