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Uncommon neo 31 EP

2010 BG2

Position computed live · sbdb

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Live ephemeris

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Score breakdown

· 6 badges
31 pts · Uncommon
Uncommon 34 pts → Rare
  • Wildly elliptical orbit +10
  • Crosses Earth's orbit +8
  • Near-Earth object +5
  • Apollo: crosses Earth's orbit +4
  • Steeply tilted orbit (i > 40°) +4
  • Catalogue designation only +0
Total score 31

3 more points to reach Rare.

Badges

  • Near-Earth object · +5
  • Wildly elliptical orbit · +10
  • Crosses Earth's orbit · +8
  • Catalogue designation only
  • Apollo: crosses Earth's orbit · +4
  • 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 Apollo-class object: its orbit is wider than Earth's but crosses it. Most known Earth-crossers belong to this family.
  • Closest approach. At its nearest it comes within 0.32 AU of the Sun — inside the orbit of Mercury.
  • One lap. A single orbit around the Sun takes it about 6.3 years.
  • How far it roams. Its orbit swings between 0.32 and 6.49 AU from the Sun.

Sense of scale

  • Sense of scale. In everyday terms it is about 3.5 football pitches across.

Standing on it

  • Sunlight there. At closest approach the Sun beats down about 10 times harder than it ever does on Earth.
  • Don't jump. Escape velocity here is only around 0.22 m/s. A determined jump would launch you off it and into your own orbit around the Sun.

Properties

aphelion au
6.49
designation
2010 BG2
eccentricity
0.9072
full name
(2010 BG2)
h mag
19.93
inclination
42.8
mean motion deg day
0.1569
moid au
0.0605
name
2010 BG2
number only
yes
orbit class
APO
perihelion au
0.316
semi major au
3.405

About 2010 BG2

2010 BG2 is an uncommon neo. It swings within 0.316 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 BG2 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 BG2 is an uncommon neo

2010 BG2 scores 31 points on Spacedle's rarity scale, which places it in the uncommon tier. Another 3 points would lift it into a rarer tier.

That score comes from 6 science badges — Near-Earth object, Wildly elliptical orbit, Crosses Earth's orbit, Catalogue designation only, Apollo: crosses Earth's orbit 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.