Skip to content
Public Universe
Asteroid Near-Earth

417210

Add to an observing list or journal →

417210 (2005 XV77)

Where is it now

Distance from Sun
1.04 AU
True anomaly
154.92°
Distance from Earth
1.077 AU
As of
16 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 — 0.997 AU from the Sun Earth 417210 — 1.04 AU from the Sun 417210
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 417210 is 1.077 AU from Earth today (9.0 light-minutes).

In the sky

Right ascension
09h 50m 06s
Declination
+17° 39′ 32″
Constellation
Leo
Distance from Earth
1.08 AU
Elongation from the Sun
60.21° — well clear of the Sun

Favours the northern hemisphere; low or below the horizon from far south.

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
0.784 AU
Eccentricity
0.4142
Inclination
16.85°
Orbital period
253.7 days
Perihelion
0.459 AU
Aphelion
1.109 AU
Longitude of ascending node
282.23°
Argument of periapsis
9.29°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 37.4 LD
0.0961 AU
Tisserand (Jupiter)
7.311

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
655
Data arc
18.08 years
First observed
10 December 2005
Last observed
10 January 2024
Residual RMS
0.42 ″
Solution · Otto Matic
25 September 2025

Visual & observation

Absolute magnitude (H)
20.55

Discovery & classification

Discovered by
CSS
Discovery date
10 December 2005
Discovery site
Catalina

Also known as 2005 XV77

Aten Near-Earth Object

Close approaches 148 on record

Flyby geometry
Ecliptic flyby of 417210 at 2030-12-24 11:03 UTC Top-down view of the ecliptic, Earth at the centre, for the 2030-12-24 11:03 UTC close approach of 417210. Catalogue miss distance 38.4 LD · 1.48 × 10⁷ km. The curve is the geocentric path from 2030-12-21 to 2030-12-27, 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 38.4 LD · 1.48 × 10⁷ km 2030-12-24 11:03 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2030-12-24 11:03 UTC close approach of 417210. Catalogue miss distance 38.4 LD · 1.48 × 10⁷ km. The curve is the geocentric path from 2030-12-21 to 2030-12-27, 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
2027-03-20 14:41:00 Mercury 0.0785 AU 30.5 LD 24.9 km/s
2027-03-20 14:41:00 Merc 0.0785 AU 30.5 LD 24.9 km/s
2030-12-24 11:03:00 Earth 0.0987 AU 38.4 LD 11.8 km/s
2032-10-12 12:11:00 Merc 0.0506 AU 19.7 LD 20.8 km/s
2032-10-12 12:11:00 Mercury 0.0506 AU 19.7 LD 20.8 km/s
2038-01-24 17:31:00 Earth 0.1597 AU 62.1 LD 11.7 km/s
2039-01-09 15:41:00 Merc 0.0397 AU 15.4 LD 22.5 km/s
2039-01-09 15:41:00 Mercury 0.0397 AU 15.4 LD 22.5 km/s
2039-12-16 17:29:00 Earth 0.1364 AU 53.1 LD 14.4 km/s
2044-08-04 07:17:00 Mercury 0.0926 AU 36.0 LD 22.3 km/s

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

Sources