Where is it now
- Distance from Sun
- 1.002 AU
- True anomaly
- 224.2°
- Distance from Earth
- 1.434 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
- 11h 01m 18s
- Declination
- +05° 39′ 31″
- Constellation
- Leo
- Distance from Earth
- 1.43 AU
- Elongation from the Sun
- 44.29° — 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.
Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.
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
- 0.911 AU
- Eccentricity
- 0.159
- Inclination
- 8.83°
- Orbital period
- 317.5 days
- Perihelion
- 0.766 AU
- Aphelion
- 1.056 AU
- Longitude of ascending node
- 295.16°
- Argument of periapsis
- 320.82°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 8.7 LD
- 0.0223 AU
- Tisserand (Jupiter)
- 6.529
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 18
- Data arc
- 7 days
- First observed
- 30 December 2024
- Last observed
- 6 January 2025
- Residual RMS
- 0.36 ″
- Solution · Otto Matic
- 7 January 2025
Visual & observation
- Absolute magnitude (H)
- 26.52
Discovery & classification
Close approaches 37 on record
Top-down view of the ecliptic, Earth at the centre, for the 2037-10-15 13:01 UTC close approach of 2024 YB26. Catalogue miss distance 61.1 LD · 2.35 × 10⁷ km. The curve is the geocentric path from 2037-10-12 to 2037-10-18, 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 |
|---|---|---|---|---|
| 2037-10-15 13:01:00 | Earth | 0.157 AU | 61.1 LD | 5.8 km/s |
| 2045-01-18 14:23:00 | Earth | 0.0299 AU | 11.6 LD | 5.9 km/s |
| 2050-08-12 19:37:00 | Venus | 0.0526 AU | 20.5 LD | 7.8 km/s |
| 2057-10-16 22:56:00 | Earth | 0.1837 AU | 71.5 LD | 7.9 km/s |
| 2061-01-26 14:35:00 | Venus | 0.0832 AU | 32.4 LD | 7.3 km/s |
| 2072-01-24 16:57:00 | Earth | 0.0692 AU | 26.9 LD | 7.7 km/s |
| 2086-04-18 04:08:00 | Venus | 0.0497 AU | 19.3 LD | 7.6 km/s |
| 2112-01-26 03:56:00 | Earth | 0.1331 AU | 51.8 LD | 9.4 km/s |
| 2115-10-31 23:59:00 | Venus | 0.1455 AU | 56.6 LD | 10.8 km/s |
| 2117-10-19 09:46:00 | Earth | 0.1798 AU | 70.0 LD | 7.6 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