Where is it now
- Distance from Sun
- 0.824 AU
- True anomaly
- 298.65°
- Distance from Earth
- 0.247 AU
- As of
- 21 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 18m 06s
- Declination
- +28° 31′ 15″
- Constellation
- Boötes
- Distance from Earth
- 0.25 AU
- Elongation from the Sun
- 40.24° — near the Sun — look low at dusk or dawn
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
- 0.912 AU
- Eccentricity
- 0.1625
- Inclination
- 22.39°
- Orbital period
- 318 days
- Perihelion
- 0.764 AU
- Aphelion
- 1.06 AU
- Longitude of ascending node
- 238.68°
- Argument of periapsis
- 210.96°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 7.5 LD
- 0.0193 AU
- Tisserand (Jupiter)
- 6.47
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 60
- Data arc
- 4 days
- First observed
- 21 May 2026
- Last observed
- 25 May 2026
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 16 June 2026
Visual & observation
- Absolute magnitude (H)
- 25.75
Discovery & classification
Close approaches 45 on record
Top-down view of the ecliptic, Earth at the centre, for the 2046-05-19 17:17 UTC close approach of 2026 KT1. Catalogue miss distance 42.4 LD · 1.63 × 10⁷ km. The curve is the geocentric path from 2046-05-16 to 2046-05-22, 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 south 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 |
|---|---|---|---|---|
| 2026-11-13 02:03:00 | Venus | 0.0551 AU | 21.5 LD | 15.9 km/s |
| 2037-04-27 15:22:00 | Venus | 0.0869 AU | 33.8 LD | 16.7 km/s |
| 2046-05-19 17:17:00 | Earth | 0.109 AU | 42.4 LD | 12.6 km/s |
| 2053-05-20 03:27:00 | Earth | 0.0923 AU | 35.9 LD | 11.2 km/s |
| 2062-07-20 18:30:00 | Venus | 0.0987 AU | 38.4 LD | 15.9 km/s |
| 2073-01-02 07:51:00 | Venus | 0.0546 AU | 21.2 LD | 16 km/s |
| 2073-05-19 05:17:00 | Earth | 0.03 AU | 11.7 LD | 11.6 km/s |
| 2080-05-20 19:34:00 | Earth | 0.1391 AU | 54.1 LD | 11.4 km/s |
| 2083-06-18 22:33:00 | Venus | 0.0594 AU | 23.1 LD | 16.1 km/s |
| 2093-12-02 02:19:00 | Venus | 0.0844 AU | 32.8 LD | 16.6 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