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Asteroid Near-Earth

Torifune

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98943 Torifune (2001 CC21)

Torifune is an asteroid in the Apollo orbit class. Its orbit takes it from 0.81 AU to 1.26 AU from the Sun; one orbit takes 383 days. Discovered 3 February 2001 by LINEAR. Orbit from the JPL solution of 30 March 2026.

Where is it now

Distance from Sun
1.138 AU
True anomaly
128.6°
Distance from Earth
0.367 AU
As of
3 November 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 — 0.992 AU from the Sun Earth Torifune — 1.138 AU from the Sun Torifune
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Torifune is 0.367 AU from Earth today (3.1 light-minutes).

In the sky

Right ascension
22h 12m 38s
Declination
-23° 26′ 35″
Constellation
Aquarius
Distance from Earth
0.37 AU
Elongation from the Sun
104.09° — well clear of the Sun

Favours the southern hemisphere; low or below the horizon from far north.

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
1.032 AU
Eccentricity
0.2192
Inclination
4.81°
Orbital period
383 days
Perihelion
0.806 AU
Aphelion
1.258 AU
Longitude of ascending node
75.36°
Argument of periapsis
179.41°
Epoch · J2000
2461200.5
Orbit class · APO
Apollo
Earth MOID · 32.3 LD
0.083 AU
Tisserand (Jupiter)
5.907

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
2,398
Data arc
43.26 years
First observed
10 November 1982
Last observed
13 February 2026
Residual RMS
0.35 ″
Solution · Davide Farnocchia
30 March 2026

Physical properties

Rotation period
5.02 hours

Visual & observation

Absolute magnitude (H)
18.71
Spectral type (SMASS)
L

Discovery & classification

Discovered by
LINEAR
Discovery date
3 February 2001
Discovery site
Socorro

Torifune (an abbreviation of Ame-no-torifune) is a god in Japanese mythology. It is also the name of the god's ship, which can travel safely at high speed like a bird and steady as a rock. The Hayabusa2 spacecraft will perform a flyby of this asteroid, and the name expresses the hope that Hayabusa2 will be able to safely conduct the high-speed encounter.

Also known as 98943 · 2001 CC21 · 1982 VE13

Apollo Near-Earth Object Named

Close approaches 67 on record

Flyby geometry
Ecliptic flyby of Torifune at 2044-03-01 15:30 UTC Sun 35.8 LD · 1.38 × 10⁷ km 2044-03-01 15:30 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2044-03-01 15:30 UTC close approach of Torifune. Catalogue miss distance 35.8 LD · 1.38 × 10⁷ km. The curve is the geocentric path from 2044-02-27 to 2044-03-04, 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. At closest approach the object is north of the ecliptic. 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
2044-03-01 15:30:00 Earth 0.0921 AU 35.8 LD 8.2 km/s
2045-05-09 20:22:00 Earth 0.194 AU 75.5 LD 7.1 km/s
2046-07-10 12:13:00 Earth 0.1934 AU 75.3 LD 7 km/s
2047-06-25 13:13:00 Venus 0.1032 AU 40.2 LD 2.2 km/s
2047-09-16 15:34:00 Earth 0.0961 AU 37.4 LD 8.4 km/s
2065-02-24 06:36:00 Earth 0.1894 AU 73.7 LD 12.2 km/s
2065-05-01 17:55:00 Venus 0.0842 AU 32.8 LD 2 km/s
2066-02-16 06:51:00 Earth 0.1608 AU 62.6 LD 4.3 km/s
2066-04-07 19:55:00 Earth 0.1518 AU 59.1 LD 5.3 km/s
2068-09-10 06:43:00 Earth 0.1044 AU 40.6 LD 5.2 km/s

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

Sources