2016 TP11 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.85 AU to 1.22 AU from the Sun; one orbit takes 385.5 days. Orbit from the JPL solution of 22 November 2022.
Where is it now
- Distance from Sun
- 1.055 AU
- True anomaly
- 254.16°
- Distance from Earth
- 1.845 AU
- As of
- 4 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
- 12h 58m 20s
- Declination
- -06° 11′ 27″
- Constellation
- Virgo
- Distance from Earth
- 1.84 AU
- Elongation from the Sun
- 26.55° — near the Sun — look low at dusk or dawn
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
- 1.037 AU
- Eccentricity
- 0.1778
- Inclination
- 1.54°
- Orbital period
- 385.5 days
- Perihelion
- 0.852 AU
- Aphelion
- 1.221 AU
- Longitude of ascending node
- 168.58°
- Argument of periapsis
- 108.2°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 3.1 LD
- 0.0081 AU
- Tisserand (Jupiter)
- 5.898
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 105
- Data arc
- 676 days
- First observed
- 18 January 2015
- Last observed
- 24 November 2016
- Residual RMS
- 0.66 ″
- Solution · Otto Matic
- 22 November 2022
Visual & observation
- Absolute magnitude (H)
- 24.3
Discovery & classification
Close approaches 66 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-03-09 20:23 UTC close approach of 2016 TP11. Catalogue miss distance 169.9 LD · 6.53 × 10⁷ km. The curve is the geocentric path from 2032-03-06 to 2032-03-12, 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 |
|---|---|---|---|---|
| 2032-03-09 20:23:00 | Earth | 0.4365 AU | 169.9 LD | 18.9 km/s |
| 2033-03-24 18:15:00 | Earth | 0.0926 AU | 36.1 LD | 8.6 km/s |
| 2034-02-06 18:19:00 | Earth | 0.1964 AU | 76.4 LD | 4.9 km/s |
| 2034-06-12 00:33:00 | Earth | 0.1612 AU | 62.7 LD | 5.5 km/s |
| 2034-12-13 15:59:00 | Earth | 0.2316 AU | 90.1 LD | 5.7 km/s |
| 2035-09-26 08:25:00 | Earth | 0.0458 AU | 17.8 LD | 4.5 km/s |
| 2036-10-11 22:18:00 | Earth | 0.2862 AU | 111.4 LD | 14.3 km/s |
| 2052-03-13 15:30:00 | Earth | 0.3323 AU | 129.3 LD | 15.8 km/s |
| 2053-03-28 06:56:00 | Moon | 0.0091 AU | 3.5 LD | 6.9 km/s |
| 2053-03-28 09:30:00 | Earth | 0.0088 AU | 3.4 LD | 5.9 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