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Asteroid Near-Earth

2010 XQ69

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(2010 XQ69)

Where is it now

Distance from Sun
1.115 AU
True anomaly
213.89°
Distance from Earth
1.719 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 2010 XQ69 — 1.115 AU from the Sun 2010 XQ69
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2010 XQ69 is 1.719 AU from Earth today (14.3 light-minutes).

In the sky

Right ascension
11h 21m 19s
Declination
+03° 39′ 27″
Constellation
Leo
Distance from Earth
1.72 AU
Elongation from the Sun
37.84° — 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
0.875 AU
Eccentricity
0.4504
Inclination
1.1°
Orbital period
299.2 days
Perihelion
0.481 AU
Aphelion
1.27 AU
Longitude of ascending node
177.39°
Argument of periapsis
105.02°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.2 LD
0.0082 AU
Tisserand (Jupiter)
6.676

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
65
Data arc
14.14 years
First observed
14 December 2010
Last observed
2 February 2025
Residual RMS
0.46 ″
Solution · Otto Matic
12 February 2025

Visual & observation

Absolute magnitude (H)
23.33

Discovery & classification

Aten Near-Earth Object

Close approaches 156 on record

Flyby geometry
Ecliptic flyby of 2010 XQ69 at 2028-11-15 07:10 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-11-15 07:10 UTC close approach of 2010 XQ69. Catalogue miss distance 14.2 LD · 5.45 × 10⁶ km. The curve is the geocentric path from 2028-11-12 to 2028-11-18, 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 south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 13 Nov 18 Nov 14.2 LD · 5.45 × 10⁶ km 2028-11-15 07:10 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-11-15 07:10 UTC close approach of 2010 XQ69. Catalogue miss distance 14.2 LD · 5.45 × 10⁶ km. The curve is the geocentric path from 2028-11-12 to 2028-11-18, 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 south 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
2028-08-28 22:50:00 Merc 0.0511 AU 19.9 LD 15.7 km/s
2028-08-28 22:50:00 Mercury 0.0511 AU 19.9 LD 15.7 km/s
2028-11-15 07:10:00 Earth 0.0364 AU 14.2 LD 12.5 km/s
2030-02-19 23:02:00 Earth 0.0407 AU 15.8 LD 14.7 km/s
2032-09-30 06:52:00 Mercury 0.0649 AU 25.3 LD 18.3 km/s
2032-09-30 06:52:00 Merc 0.0649 AU 25.3 LD 18.3 km/s
2036-11-01 12:25:00 Mercury 0.0965 AU 37.5 LD 22.1 km/s
2036-11-01 12:25:00 Merc 0.0965 AU 37.5 LD 22.1 km/s
2037-11-15 18:16:00 Earth 0.046 AU 17.9 LD 12.2 km/s
2039-02-19 17:18:00 Earth 0.0608 AU 23.6 LD 15.4 km/s

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

Sources