Where is it now
- Distance from Sun
- 0.924 AU
- True anomaly
- 130.78°
- Distance from Earth
- 1.048 AU
- As of
- 17 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
- 17h 13m 20s
- Declination
- -12° 17′ 30″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.05 AU
- Elongation from the Sun
- 53.86° — 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
- 0.817 AU
- Eccentricity
- 0.2907
- Inclination
- 15.66°
- Orbital period
- 269.9 days
- Perihelion
- 0.58 AU
- Aphelion
- 1.055 AU
- Longitude of ascending node
- 189.72°
- Argument of periapsis
- 357.37°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 20.8 LD
- 0.0533 AU
- Tisserand (Jupiter)
- 7.096
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 82
- Data arc
- 21 days
- First observed
- 3 October 2024
- Last observed
- 24 October 2024
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 24 October 2024
Visual & observation
- Absolute magnitude (H)
- 23.84
Discovery & classification
Close approaches 81 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-05-24 20:02 UTC close approach of 2024 TY1. Catalogue miss distance 158.6 LD · 6.1 × 10⁷ km. The curve is the geocentric path from 2027-05-21 to 2027-05-27, 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 a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2027-05-24 20:02:00 | Earth | 0.4075 AU | 158.6 LD | 13.2 km/s |
| 2027-10-23 16:08:00 | Earth | 0.2364 AU | 92.0 LD | 13.5 km/s |
| 2029-07-19 21:53:00 | Venus | 0.1428 AU | 55.6 LD | 15 km/s |
| 2030-04-23 08:28:00 | Earth | 0.4201 AU | 163.5 LD | 16.8 km/s |
| 2030-10-19 01:21:00 | Earth | 0.4723 AU | 183.8 LD | 21.2 km/s |
| 2033-03-25 19:08:00 | Earth | 0.4181 AU | 162.7 LD | 17.6 km/s |
| 2033-03-31 23:49:00 | Venus | 0.1395 AU | 54.3 LD | 15 km/s |
| 2035-09-12 15:52:00 | Earth | 0.3395 AU | 132.1 LD | 16.7 km/s |
| 2036-02-25 15:16:00 | Earth | 0.4073 AU | 158.5 LD | 15.8 km/s |
| 2036-12-12 04:08:00 | Venus | 0.1371 AU | 53.4 LD | 14.9 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