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Rare neo 35 EP

2010 GV147

Position computed live · sbdb

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Live ephemeris

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Score breakdown

· 6 badges
35 pts · Rare
Rare 50 pts → Epic
  • Darker than charcoal +10
  • Crosses Earth's orbit +8
  • Aten: mostly inside Earth's orbit +8
  • Near-Earth object +5
  • Steeply tilted orbit (i > 40°) +4
  • Catalogue designation only +0
Total score 35

15 more points to reach Epic.

Badges

  • Near-Earth object · +5
  • Crosses Earth's orbit · +8
  • Catalogue designation only
  • Aten: mostly inside Earth's orbit · +8
  • Darker than charcoal · +10
  • Steeply tilted orbit (i > 40°) · +4

Trivia

What makes it special

  • It crosses our path. Its orbit genuinely intersects Earth's track around the Sun. The two paths cross; only the timing keeps them apart.

What it actually is

  • Its orbit family. An Aten-class object, spending most of its time inside Earth's orbit and crossing ours from the sunward side — which makes this family wretchedly hard to spot against the daylight.
  • Closest approach. At its nearest it comes within 0.33 AU of the Sun — inside the orbit of Mercury.
  • One lap. A single orbit around the Sun takes it about 343 days.
  • How far it roams. Its orbit swings between 0.33 and 1.59 AU from the Sun.

Sense of scale

  • Sense of scale. In everyday terms it is roughly 0.2× the height of Mount Everest.

Standing on it

  • Sunlight there. At closest approach the Sun beats down about 9.4 times harder than it ever does on Earth.
  • Don't jump. Escape velocity here is only around 1.24 m/s. A determined jump would launch you off it and into your own orbit around the Sun.

Properties

albedo
0.018
aphelion au
1.59
designation
2010 GV147
diameter km
2.055
eccentricity
0.6602
full name
(2010 GV147)
h mag
18.29
inclination
44.05
mean motion deg day
1.05
moid au
0.317
name
2010 GV147
number only
yes
orbit class
ATE
perihelion au
0.326
semi major au
0.9588

About 2010 GV147

2010 GV147 is a rare neo. It swings within 0.326 AU of the Sun at perihelion.

Its orbit genuinely intersects Earth's track around the Sun. The two paths cross; only the timing keeps them apart.

How to see it

Like any astronomical target, 2010 GV147 is best seen from a dark site away from city lights, and when it is above the horizon depends on your latitude and the time of year. Because it moves against the background stars, the live position panel on this page tracks where it is right now. The visibility panel above works out tonight's viewing window for your saved location.

Why 2010 GV147 is a rare neo

2010 GV147 scores 35 points on Spacedle's rarity scale, which places it in the rare tier. Another 15 points would lift it into a rarer tier.

That score comes from 6 science badges — Near-Earth object, Crosses Earth's orbit, Catalogue designation only, Aten: mostly inside Earth's orbit, Darker than charcoal and Steeply tilted orbit (i > 40°) — each earned for a real, measurable property of the object. Rarity on Spacedle is never random: the more remarkable an object's astrophysics, the more badges it collects, the higher it scores, and the rarer it ranks.