2024 XT49 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 34.2 AU to 62.21 AU from the Sun; one orbit takes 334.7 years. Orbit from the JPL solution of 11 March 2026.
Where is it now
- Distance from Sun
- 61.224 AU
- True anomaly
- 196.12°
- Distance from Earth
- 60.327 AU
- As of
- 26 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
- 03h 47m 48s
- Declination
- +19° 44′ 29″
- Constellation
- Taurus
- Distance from Earth
- 60.33 AU
- Elongation from the Sun
- 154.29° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
From your location
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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
- 48.203 AU
- Eccentricity
- 0.2906
- Inclination
- 9.17°
- Orbital period
- 334.7 years
- Perihelion
- 34.196 AU
- Aphelion
- 62.21 AU
- Longitude of ascending node
- 237.34°
- Argument of periapsis
- 345.27°
- Epoch · J2000
- 2460766.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 12,916.0 LD
- 33.1884 AU
- Tisserand (Jupiter)
- 5.858
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 9).
- Observations used
- 6
- Data arc
- 385 days
- First observed
- 3 December 2024
- Last observed
- 23 December 2025
- Residual RMS
- 0.09 ″
- Solution · Otto Matic
- 11 March 2026
Visual & observation
- Absolute magnitude (H)
- 7.41
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB