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Rare neo 35 EP

(345705) 2006 VB14

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
  • Brilliantly reflective surface +10
  • Crosses Earth's orbit +8
  • Aten: mostly inside Earth's orbit +8
  • Near-Earth object +5
  • Tiny fragment (<1 km) +4
  • Catalogue designation only +0
Total score 35

15 more points to reach Epic.

Badges

  • Near-Earth object · +5
  • Tiny fragment (<1 km) · +4
  • Crosses Earth's orbit · +8
  • Catalogue designation only
  • Aten: mostly inside Earth's orbit · +8
  • Brilliantly reflective surface · +10

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 0.44 AU of the Sun — inside the orbit of Venus.
  • One lap. A single orbit around the Sun takes it about 245 days.
  • How far it roams. Its orbit swings between 0.44 and 1.09 AU from the Sun.

Sense of scale

  • Sense of scale. In everyday terms it is about 3.9 football pitches across.

Standing on it

  • Sunlight there. At closest approach the Sun beats down about 5.1 times harder than it ever does on Earth.
  • Don't jump. Escape velocity here is only around 0.24 m/s. A determined jump would launch you off it and into your own orbit around the Sun.

Properties

albedo
0.402
aphelion au
1.09
designation
345705
diameter km
0.406
eccentricity
0.4211
full name
345705 (2006 VB14)
h mag
18.58
inclination
31.03
mean motion deg day
1.467
moid au
0.0783
name
(345705) 2006 VB14
number only
yes
orbit class
ATE
perihelion au
0.444
rotation period h
3.204
semi major au
0.767

About (345705) 2006 VB14

(345705) 2006 VB14 is a rare neo. It swings within 0.444 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, (345705) 2006 VB14 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 (345705) 2006 VB14 is a rare neo

(345705) 2006 VB14 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, Tiny fragment (<1 km), Crosses Earth's orbit, Catalogue designation only, Aten: mostly inside Earth's orbit and Brilliantly reflective surface — 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.