2026 DL19 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.68 AU to 1.39 AU from the Sun; one orbit takes 384.4 days. Orbit from the JPL solution of 19 March 2026.
Where is it now
- Distance from Sun
- 1.385 AU
- True anomaly
- 172.83°
- Distance from Earth
- 0.868 AU
- As of
- 3 November 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
- 08h 56m 06s
- Declination
- +39° 12′ 28″
- Constellation
- Lynx
- Distance from Earth
- 0.86 AU
- Elongation from the Sun
- 96.59° — 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
- 1.035 AU
- Eccentricity
- 0.3442
- Inclination
- 12.97°
- Orbital period
- 384.4 days
- Perihelion
- 0.679 AU
- Aphelion
- 1.391 AU
- Longitude of ascending node
- 340.82°
- Argument of periapsis
- 284.16°
- Epoch · J2000
- 2461099.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.0 LD
- 0.0025 AU
- Tisserand (Jupiter)
- 5.845
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 18
- Data arc
- 24 hours
- First observed
- 27 February 2026
- Last observed
- 28 February 2026
- Residual RMS
- 0.36 ″
- Solution · Otto Matic
- 19 March 2026
Visual & observation
- Absolute magnitude (H)
- 28.76
Discovery & classification
Close approaches 9 on record
Top-down view of the ecliptic, Earth at the centre, for the 2030-10-04 09:43 UTC close approach of 2026 DL19. Catalogue miss distance 76.1 LD · 2.92 × 10⁷ km. The curve is the geocentric path from 2030-10-01 to 2030-10-07, 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 |
|---|---|---|---|---|
| 2028-07-18 14:06:00 | Venus | 0.1186 AU | 46.2 LD | 16.6 km/s |
| 2030-10-04 09:43:00 | Earth | 0.1955 AU | 76.1 LD | 17.4 km/s |
| 2065-09-23 15:26:00 | Earth | 0.0905 AU | 35.2 LD | 12.6 km/s |
| 2079-02-27 11:51:00 | Earth | 0.0884 AU | 34.4 LD | 15.2 km/s |
| 2104-10-30 07:07:00 | Venus | 0.0948 AU | 36.9 LD | 15.6 km/s |
| 2176-10-16 11:00:00 | Venus | 0.0456 AU | 17.7 LD | 11.6 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