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Asteroid Near-Earth

2017 CP32

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(2017 CP32)

Where is it now

Distance from Sun
0.721 AU
True anomaly
291.68°
Distance from Earth
1.257 AU
As of
19 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 — 0.996 AU from the Sun Earth 2017 CP32 — 0.721 AU from the Sun 2017 CP32
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2017 CP32 is 1.257 AU from Earth today (10.5 light-minutes).

In the sky

Right ascension
15h 53m 02s
Declination
-25° 10′ 45″
Constellation
Scorpius
Distance from Earth
1.25 AU
Elongation from the Sun
34.98° — near the Sun — look low at dusk or dawn

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
0.841 AU
Eccentricity
0.2516
Inclination
17°
Orbital period
281.8 days
Perihelion
0.63 AU
Aphelion
1.053 AU
Longitude of ascending node
323.32°
Argument of periapsis
37.48°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.9 LD
0.0023 AU
Tisserand (Jupiter)
6.931

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
47
Data arc
15 days
First observed
15 February 2017
Last observed
2 March 2017
Residual RMS
0.31 ″
Solution · Otto Matic
15 April 2021

Physical properties

Rotation period
1.7 hours

Visual & observation

Absolute magnitude (H)
24.01

Discovery & classification

Aten Near-Earth Object

Close approaches 70 on record

Flyby geometry
Ecliptic flyby of 2017 CP32 at 2027-02-14 23:58 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-02-14 23:58 UTC close approach of 2017 CP32. Catalogue miss distance 81.1 LD · 3.12 × 10⁷ km. The curve is the geocentric path from 2027-02-11 to 2027-02-17, 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 81.1 LD · 3.12 × 10⁷ km 2027-02-14 23:58 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-02-14 23:58 UTC close approach of 2017 CP32. Catalogue miss distance 81.1 LD · 3.12 × 10⁷ km. The curve is the geocentric path from 2027-02-11 to 2027-02-17, 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
2027-02-14 23:58:00 Earth 0.2083 AU 81.1 LD 14.9 km/s
2027-08-05 07:18:00 Earth 0.3413 AU 132.8 LD 14.2 km/s
2029-02-20 03:13:00 Venus 0.0576 AU 22.4 LD 13.6 km/s
2030-10-05 09:19:00 Earth 0.4081 AU 158.8 LD 14.3 km/s
2031-04-12 01:00:00 Earth 0.4726 AU 183.9 LD 17.7 km/s
2032-03-27 17:14:00 Venus 0.1107 AU 43.1 LD 13 km/s
2034-02-17 22:30:00 Earth 0.1098 AU 42.7 LD 9.2 km/s
2034-06-19 08:59:00 Earth 0.3086 AU 120.1 LD 10.1 km/s
2037-02-20 06:44:00 Earth 0.3909 AU 152.1 LD 20.1 km/s
2037-08-26 13:49:00 Earth 0.3683 AU 143.4 LD 15.3 km/s

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

Sources