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Common neo 21 EP

(2002 AO11)

Position computed live · sbdb

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Live ephemeris

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Score breakdown

· 4 badges
21 pts · Common
Common 24 pts → Uncommon
  • Crosses Earth's orbit +12
  • Near-Earth object +5
  • Tiny fragment (<1 km) +4
  • Catalogue designation only +0
Total score 21

3 more points to reach Uncommon.

Badges

  • Near-Earth object · +5
  • Tiny fragment (<1 km) · +4
  • Crosses Earth's orbit · +12
  • Catalogue designation only

Trivia

How we found it

  • Designation. Known only by its catalogue designation — no name yet.

Cosmic context

  • Size. Roughly 0.2 km across.
  • Ancient. A leftover from the Solar System's birth, older than every continent on Earth.

Properties

diameter km
0.175
eccentricity
0.1621
h mag
23.05
inclination
13.06
name
(2002 AO11)
number only
yes
orbit class
ATE
perihelion au
0.7685
semi major au
0.9172

About (2002 AO11)

(2002 AO11) is a common neo. It swings within 0.769 AU of the Sun at perihelion.

Roughly 0.2 km across.

How to see it

Like any astronomical target, (2002 AO11) 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 (2002 AO11) is a common neo

(2002 AO11) scores 21 points on Spacedle's rarity scale, which places it in the common tier. Another 3 points would lift it into a rarer tier.

That score comes from 4 science badges — Near-Earth object, Tiny fragment (<1 km), Crosses Earth's orbit and Catalogue designation only — 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.

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Sky imagery and survey data courtesy of Aladin Lite & CDS, Strasbourg. Object data from the NASA Exoplanet Archive, JPL Small-Body Database, and the ATNF Pulsar Catalogue.