2014 TW is an asteroid in the Amor orbit class. Its orbit takes it from 1.02 AU to 1.04 AU from the Sun; one orbit takes 381.2 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.02 AU
- True anomaly
- 16.74°
- Distance from Earth
- 2.01 AU
- As of
- 3 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
- 14h 28m 58s
- Declination
- -16° 58′ 13″
- Constellation
- Libra
- Distance from Earth
- 2.01 AU
- Elongation from the Sun
- 2.78° — too close to the Sun to observe
Favours the southern hemisphere; low or below the horizon from far north.
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
- 1.029 AU
- Eccentricity
- 0.0087
- Inclination
- 9.01°
- Orbital period
- 381.2 days
- Perihelion
- 1.02 AU
- Aphelion
- 1.038 AU
- Longitude of ascending node
- 10.76°
- Argument of periapsis
- 190.68°
- Epoch · J2000
- 2461200.5
- Orbit class · AMO
- Amor
- Earth MOID · 8.2 LD
- 0.0211 AU
- Tisserand (Jupiter)
- 5.936
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 51
- Data arc
- 29 days
- First observed
- 2 October 2014
- Last observed
- 31 October 2014
- Residual RMS
- 0.84 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.06
Discovery & classification
Close approaches 41 on record
Top-down view of the ecliptic, Earth at the centre, for the 2037-04-07 12:39 UTC close approach of 2014 TW. Catalogue miss distance 119.6 LD · 4.6 × 10⁷ km. The curve is the geocentric path from 2037-04-04 to 2037-04-10, 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 |
|---|---|---|---|---|
| 2037-04-07 12:39:00 | Earth | 0.3074 AU | 119.6 LD | 10.4 km/s |
| 2038-04-02 20:52:00 | Earth | 0.0463 AU | 18.0 LD | 5 km/s |
| 2038-10-02 01:27:00 | Earth | 0.0342 AU | 13.3 LD | 4.7 km/s |
| 2039-03-19 19:55:00 | Earth | 0.2044 AU | 79.5 LD | 6.9 km/s |
| 2039-09-15 00:35:00 | Earth | 0.2559 AU | 99.6 LD | 8.7 km/s |
| 2061-04-11 18:00:00 | Earth | 0.4786 AU | 186.3 LD | 14.9 km/s |
| 2062-04-07 16:16:00 | Earth | 0.2234 AU | 86.9 LD | 8.3 km/s |
| 2062-10-21 07:58:00 | Earth | 0.1587 AU | 61.8 LD | 5.8 km/s |
| 2063-03-31 10:38:00 | Earth | 0.0377 AU | 14.7 LD | 4.7 km/s |
| 2063-09-24 18:21:00 | Earth | 0.0951 AU | 37.0 LD | 5.5 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