137427
Add to an observing list or journal →137427 (1999 TF211)
Where is it now
- Distance from Sun
- 2.025 AU
- True anomaly
- 246.26°
- Distance from Earth
- 1.268 AU
- As of
- 11 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
- 00h 42m 36s
- Declination
- +60° 57′ 36″
- Constellation
- Cassiopeia
- Distance from Earth
- 1.26 AU
- Elongation from the Sun
- 126.25° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 2.439 AU
- Eccentricity
- 0.6119
- Inclination
- 39.51°
- Orbital period
- 3.81 years
- Perihelion
- 0.947 AU
- Aphelion
- 3.932 AU
- Longitude of ascending node
- 347.9°
- Argument of periapsis
- 162.4°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 11.0 LD
- 0.0283 AU
- Tisserand (Jupiter)
- 2.969
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 927
- Data arc
- 27 years
- First observed
- 6 October 1999
- Last observed
- 6 October 2026
- Residual RMS
- 0.57 ″
- Solution · Otto Matic
- 7 October 2026
Visual & observation
- Absolute magnitude (H)
- 15.28
Discovery & classification
- Discovered by
- LINEAR
- Discovery date
- 15 October 1999
- Discovery site
- Socorro
Also known as 1999 TF211
Close approaches 16 on record
Top-down view of the ecliptic, Earth at the centre, for the 2065-03-03 19:20 UTC close approach of 137427. Catalogue miss distance 36.7 LD · 1.41 × 10⁷ km. The curve is the geocentric path from 2065-02-28 to 2065-03-06, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2065-03-03 19:20:00 | Earth | 0.0943 AU | 36.7 LD | 24.7 km/s |
| 2093-07-29 07:04:00 | Juptr | 1.861 AU | 724.2 LD | 9.8 km/s |
| 2103-02-28 02:09:00 | Earth | 0.1775 AU | 69.1 LD | 24.2 km/s |
| 2105-03-31 02:30:00 | Juptr | 1.2694 AU | 494.0 LD | 8.8 km/s |
| 2116-11-22 14:50:00 | Juptr | 1.232 AU | 479.5 LD | 9.4 km/s |
| 2128-06-27 06:48:00 | Juptr | 1.7906 AU | 696.8 LD | 11.1 km/s |
| 2179-03-02 16:17:00 | Earth | 0.1298 AU | 50.5 LD | 24.5 km/s |
| 2198-03-05 21:13:00 | Earth | 0.0693 AU | 27.0 LD | 24.3 km/s |
| 2200-03-10 20:21:00 | Juptr | 1.3492 AU | 525.1 LD | 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