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Asteroid Near-Earth

2006 SP19

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(2006 SP19)

Where is it now

Distance from Sun
0.784 AU
True anomaly
275.42°
Distance from Earth
0.811 AU
As of
20 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.

Sun Earth — 0.996 AU from the Sun Earth 2006 SP19 — 0.784 AU from the Sun 2006 SP19
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2006 SP19 is 0.811 AU from Earth today (6.7 light-minutes).

In the sky

Right ascension
10h 44m 25s
Declination
+12° 43′ 01″
Constellation
Leo
Distance from Earth
0.81 AU
Elongation from the Sun
50.02° — 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.

How do I find my coordinates?

Google Maps on a computer

  1. Right-click the spot where you'll be observing.
  2. The first line of the menu is the coordinates, e.g. 51.50722, -0.12758 — click it and they're copied.
  3. Paste them above.

Google Maps on a phone

  1. Press and hold the spot to drop a pin.
  2. The coordinates appear in the search bar (or on the pin's card) — tap to copy, then paste above.

A full Google Maps link works too, but the short maps.app.goo.gl share links don't carry coordinates — copy the numbers instead. We round to about a kilometre; that's all the sky calculation needs.

Know your what3words address? Paste it, e.g. ///filled.count.soap. This is optional — the three words are sent to what3words to convert them, and we don't store the address or the result.

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
0.881 AU
Eccentricity
0.293
Inclination
4.59°
Orbital period
302.1 days
Perihelion
0.623 AU
Aphelion
1.139 AU
Longitude of ascending node
357.88°
Argument of periapsis
166.54°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 17.8 LD
0.0458 AU
Tisserand (Jupiter)
6.69

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
51
Data arc
18.99 years
First observed
19 September 2006
Last observed
16 September 2025
Residual RMS
0.89 ″
Solution · Otto Matic
25 August 2026

Visual & observation

Absolute magnitude (H)
24.22

Discovery & classification

Aten Near-Earth Object

Close approaches 108 on record

Flyby geometry
Ecliptic flyby of 2006 SP19 at 2030-10-24 21:26 UTC Top-down view of the ecliptic, Earth at the centre, for the 2030-10-24 21:26 UTC close approach of 2006 SP19. Catalogue miss distance 18.2 LD · 6.98 × 10⁶ km. The curve is the geocentric path from 2030-10-21 to 2030-10-27, 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. Sun 22 Oct 27 Oct 18.2 LD · 6.98 × 10⁶ km 2030-10-24 21:26 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2030-10-24 21:26 UTC close approach of 2006 SP19. Catalogue miss distance 18.2 LD · 6.98 × 10⁶ km. The curve is the geocentric path from 2030-10-21 to 2030-10-27, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2030-10-24 21:26:00 Earth 0.0467 AU 18.2 LD 7.5 km/s
2036-10-03 04:22:00 Venus 0.1169 AU 45.5 LD 14.4 km/s
2039-04-01 20:04:00 Venus 0.044 AU 17.1 LD 8.3 km/s
2039-07-23 20:40:00 Earth 0.1061 AU 41.3 LD 10.1 km/s
2041-10-20 05:30:00 Venus 0.1 AU 38.9 LD 8.3 km/s
2044-05-14 06:33:00 Venus 0.0705 AU 27.4 LD 7.7 km/s
2044-08-18 01:50:00 Earth 0.1189 AU 46.3 LD 6.2 km/s
2046-11-10 20:38:00 Venus 0.1328 AU 51.7 LD 14.6 km/s
2049-10-06 08:57:00 Earth 0.1032 AU 40.2 LD 6.2 km/s
2054-10-26 12:53:00 Earth 0.0998 AU 38.9 LD 10.4 km/s

Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.

Sources