2018 RY7 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.87 AU to 1.17 AU from the Sun; one orbit takes 374.5 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.158 AU
- True anomaly
- 196.91°
- Distance from Earth
- 1.156 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.
In the sky
- Right ascension
- 19h 13m 49s
- Declination
- -28° 12′ 44″
- Constellation
- Sagittarius
- Distance from Earth
- 1.16 AU
- Elongation from the Sun
- 64.64° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
From your location
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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
- 1.017 AU
- Eccentricity
- 0.1472
- Inclination
- 13.35°
- Orbital period
- 374.5 days
- Perihelion
- 0.867 AU
- Aphelion
- 1.167 AU
- Longitude of ascending node
- 2.69°
- Argument of periapsis
- 136.74°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 36.2 LD
- 0.093 AU
- Tisserand (Jupiter)
- 5.968
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 97
- Data arc
- 329 days
- First observed
- 14 September 2018
- Last observed
- 9 August 2019
- Residual RMS
- 0.34 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.4
Discovery & classification
Close approaches 87 on record
Top-down view of the ecliptic, Earth at the centre, for the 2055-10-13 07:05 UTC close approach of 2018 RY7. Catalogue miss distance 193.8 LD · 7.45 × 10⁷ km. The curve is the geocentric path from 2055-10-10 to 2055-10-16, 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.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2055-10-13 07:05:00 | Earth | 0.498 AU | 193.8 LD | 19.1 km/s |
| 2056-10-16 15:23:00 | Earth | 0.3519 AU | 137.0 LD | 14.7 km/s |
| 2057-10-17 19:11:00 | Earth | 0.2145 AU | 83.5 LD | 10.9 km/s |
| 2058-10-12 10:16:00 | Earth | 0.1129 AU | 43.9 LD | 8.2 km/s |
| 2059-09-28 20:09:00 | Earth | 0.1197 AU | 46.6 LD | 7.3 km/s |
| 2060-02-11 12:07:00 | Earth | 0.2036 AU | 79.2 LD | 7.8 km/s |
| 2060-09-08 07:41:00 | Earth | 0.1911 AU | 74.4 LD | 7.3 km/s |
| 2061-03-15 06:46:00 | Earth | 0.1212 AU | 47.2 LD | 8 km/s |
| 2061-08-11 11:38:00 | Earth | 0.2546 AU | 99.1 LD | 6.6 km/s |
| 2062-04-09 03:00:00 | Earth | 0.1042 AU | 40.6 LD | 8.6 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB