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Asteroid Near-Earth

96590

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96590 (1998 XB)

Where is it now

Distance from Sun
0.992 AU
True anomaly
235.8°
Distance from Earth
1.758 AU
As of
21 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 96590 — 0.992 AU from the Sun 96590
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 96590 is 1.758 AU from Earth today (14.6 light-minutes).

In the sky

Right ascension
12h 17m 41s
Declination
+06° 13′ 40″
Constellation
Virgo
Distance from Earth
1.76 AU
Elongation from the Sun
27.72° — near the Sun — look low at dusk or dawn

Visible from both hemispheres.

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
0.908 AU
Eccentricity
0.3512
Inclination
13.6°
Orbital period
316 days
Perihelion
0.589 AU
Aphelion
1.227 AU
Longitude of ascending node
75.68°
Argument of periapsis
202.72°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 44.2 LD
0.1136 AU
Tisserand (Jupiter)
6.492

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
3,847
Data arc
33.85 years
First observed
1 January 1992
Last observed
8 November 2025
Residual RMS
0.44 ″
Solution · Otto Matic
16 June 2026

Physical properties

Mean radius
0.44 km
Rotation period
21.67 days

Visual & observation

Geometric albedo
0.489
Absolute magnitude (H)
16.28
Spectral type (SMASS)
S:

Discovery & classification

Discovered by
Beijing Schmidt CCD Asteroid Program
Discovery date
1 December 1998
Discovery site
Xinglong

Also known as 1998 XB

Aten Near-Earth Object

Close approaches 68 on record

Flyby geometry
Ecliptic flyby of 96590 at 2029-11-28 15:13 UTC Top-down view of the ecliptic, Earth at the centre, for the 2029-11-28 15:13 UTC close approach of 96590. Catalogue miss distance 70.9 LD · 2.72 × 10⁷ km. The curve is the geocentric path from 2029-11-25 to 2029-12-01, 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 70.9 LD · 2.72 × 10⁷ km 2029-11-28 15:13 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2029-11-28 15:13 UTC close approach of 96590. Catalogue miss distance 70.9 LD · 2.72 × 10⁷ km. The curve is the geocentric path from 2029-11-25 to 2029-12-01, 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
2027-12-10 05:11:00 Venus 0.1414 AU 55.0 LD 9.7 km/s
2029-11-28 15:13:00 Earth 0.1821 AU 70.9 LD 10.1 km/s
2032-04-18 00:21:00 Venus 0.1429 AU 55.6 LD 14.7 km/s
2035-11-13 21:59:00 Earth 0.1722 AU 67.0 LD 15.2 km/s
2042-07-04 16:11:00 Venus 0.0882 AU 34.3 LD 12.8 km/s
2046-11-13 17:05:00 Venus 0.1184 AU 46.1 LD 11.7 km/s
2048-11-14 04:34:00 Earth 0.1136 AU 44.2 LD 11.7 km/s
2051-03-27 09:59:00 Venus 0.1487 AU 57.9 LD 12.1 km/s
2055-08-12 06:53:00 Venus 0.1454 AU 56.6 LD 10 km/s
2059-12-23 16:04:00 Venus 0.1372 AU 53.4 LD 14 km/s

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

Sources