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Asteroid Near-Earth

2015 BM510

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(2015 BM510)

Where is it now

Distance from Sun
1.036 AU
True anomaly
144.53°
Distance from Earth
0.366 AU
As of
22 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 — 0.995 AU from the Sun Earth 2015 BM510 — 1.036 AU from the Sun 2015 BM510
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2015 BM510 is 0.366 AU from Earth today (3.0 light-minutes).

In the sky

Right ascension
08h 26m 14s
Declination
+22° 01′ 16″
Constellation
Cancer
Distance from Earth
0.37 AU
Elongation from the Sun
86.11° — 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
0.948 AU
Eccentricity
0.1212
Inclination
1.59°
Orbital period
337 days
Perihelion
0.833 AU
Aphelion
1.063 AU
Longitude of ascending node
267.65°
Argument of periapsis
357.77°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 9.3 LD
0.0238 AU
Tisserand (Jupiter)
6.337

Orbit quality

Orbit very well determined (uncertainty code 1).

Observations used
68
Data arc
23.01 years
First observed
14 November 2002
Last observed
16 November 2025
Residual RMS
0.31 ″
Solution · Otto Matic
25 November 2025

Physical properties

Rotation period
0.81 hours

Visual & observation

Absolute magnitude (H)
25.04

Discovery & classification

Aten Near-Earth Object

Close approaches 83 on record

Flyby geometry
Ecliptic flyby of 2015 BM510 at 2027-02-17 02:54 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-02-17 02:54 UTC close approach of 2015 BM510. Catalogue miss distance 43.2 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2027-02-14 to 2027-02-20, 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. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 43.2 LD · 1.66 × 10⁷ km 2027-02-17 02:54 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-02-17 02:54 UTC close approach of 2015 BM510. Catalogue miss distance 43.2 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2027-02-14 to 2027-02-20, 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. 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
2027-02-17 02:54:00 Earth 0.1111 AU 43.2 LD 7.1 km/s
2037-10-27 14:58:00 Earth 0.038 AU 14.8 LD 3.1 km/s
2038-05-18 02:34:00 Earth 0.172 AU 66.9 LD 4.9 km/s
2049-07-20 10:55:00 Earth 0.1725 AU 67.1 LD 4.8 km/s
2050-02-08 18:38:00 Earth 0.0375 AU 14.6 LD 3.1 km/s
2060-10-18 19:41:00 Earth 0.116 AU 45.1 LD 7.3 km/s
2061-06-23 05:35:00 Earth 0.183 AU 71.2 LD 5.3 km/s
2062-02-16 09:04:00 Earth 0.0745 AU 29.0 LD 6 km/s
2072-10-23 01:23:00 Earth 0.0307 AU 11.9 LD 3.3 km/s
2073-05-19 10:57:00 Earth 0.1745 AU 67.9 LD 5 km/s

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

Sources