2026 TV is an asteroid in the Aten orbit class. Its orbit takes it from 0.49 AU to 1.47 AU from the Sun; one orbit takes 354.9 days. Orbit from the JPL solution of 9 October 2026.
Where is it now
- Distance from Sun
- 1.254 AU
- True anomaly
- 145.76°
- Distance from Earth
- 0.362 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
- 23h 18m 04s
- Declination
- -00° 35′ 32″
- Constellation
- Pisces
- Distance from Earth
- 0.37 AU
- Elongation from the Sun
- 129.3° — 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
- 0.981 AU
- Eccentricity
- 0.4996
- Inclination
- 3.34°
- Orbital period
- 354.9 days
- Perihelion
- 0.491 AU
- Aphelion
- 1.471 AU
- Longitude of ascending node
- 226.07°
- Argument of periapsis
- 15.65°
- Epoch · J2000
- 2461316.5
- Orbit class · ATE
- Aten
- Earth MOID · 15.3 LD
- 0.0392 AU
- Tisserand (Jupiter)
- 6.055
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 42
- Data arc
- 5 days
- First observed
- 3 October 2026
- Last observed
- 8 October 2026
- Residual RMS
- 0.29 ″
- Solution · Otto Matic
- 9 October 2026
Visual & observation
- Absolute magnitude (H)
- 24.2
Discovery & classification
Close approaches 8 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-27 05:52 UTC close approach of 2026 TV. Catalogue miss distance 67.2 LD · 2.58 × 10⁷ km. The curve is the geocentric path from 2027-09-24 to 2027-09-30, 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 |
|---|---|---|---|---|
| 2027-09-27 05:52:00 | Earth | 0.1727 AU | 67.2 LD | 11.3 km/s |
| 2031-05-03 06:18:00 | Venus | 0.0867 AU | 33.7 LD | 15.9 km/s |
| 2037-01-22 10:41:00 | Earth | 0.1685 AU | 65.6 LD | 11.3 km/s |
| 2038-01-21 10:39:00 | Earth | 0.0572 AU | 22.2 LD | 16.2 km/s |
| 2142-01-21 14:20:00 | Venus | 0.1135 AU | 44.2 LD | 21.3 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