
Image by Leo_65 on Pixabay · Pixabay License
OverviewAI-generated
381 Myrrha is a C-type asteroid located in the asteroid belt, orbiting the Sun. It was discovered on January 10, 1894, by Auguste Charlois at the Nice Observatory. The minor planet is named after Myrrha and holds the provisional designations 1894 AS and A894 AC. In the sequence of numbered asteroids, it follows 380 Fiducia and is followed by 382 Dodona.
Physically, 381 Myrrha has a diameter of 127.639 kilometers and an albedo of 0.064. Its rotation period is 6.572 hours, and its absolute magnitude is 8.38. The asteroid is classified as an Outer Main-belt Asteroid.
Orbitally, the object has a semi-major axis of 3.234105578029831 astronomical units. Its orbital eccentricity is 0.08789247842360084, with a periapsis of 2.949852023293197 and an apoapsis of 3.518359132766465. The orbital inclination is 12.6099828639309 degrees, and the longitude of the ascending node is 124.7153787120321 degrees.
Synthesized by Vinony from 35 facts across 4 sources: Wikidata, NASA, Jpl Sbdb, Vinony graph. Generated from structured data (not the Wikipedia text) and checked against those facts — may still contain errors.
Picture of the Day · NASA

Pathfinder on Mars
2026-07-04
On July 4th, 1997, using its own array of fireworks, a parachute, and a cocoon of airbags, the Mars Pathfinder spacecraft bounced like a giant beach ball at least 15 times before it came to rest on the surface of Mars at 10:07 AM Pacific Daylight Time. After its then novel airbag-assisted landing sequence was completed, Pathfinder transmitted this color mosaic to mission operators on Earth. In the scene from another world, the Mars Sojourner robot rover is visible in the foreground, crouched on top of the unfolded Pathfinder. About the size of a large house cat, the six-wheeled, solar-powered Sojourner became the first successful Martian rover. Surrounding Pathfinder are deflated airbags and the rock-strewn terrain of the Ares Vallis floodplain. In the distance Martian hills appear against a dusty brownish sky. The Pathfinder lander was subsequently renamed the Carl Sagan Memorial Station.
via NASA APOD
Small body data
381 Myrrha (A894 AC)
- Orbit class
- Outer Main-belt Asteroid
- Diameter
- 127.639 km
- Albedo
- 0.064
- Rotation period
- 6.572 h
- Absolute magnitude
- 8.380 H
- Earth MOID
- 1.940 AU
via NASA/JPL Small-Body Database
Key facts
- Discovered by
- Auguste Charlois
- Discovery date
- 10 January 1894
- Pronunciation
- / ˈ m ɪr ə , ˈ m ɜːr ə /
- Named after
- Myrrha
- Alternative designations
- 1894 AS
- Minor planet category
- Main belt
- Observation arc
- 122.27 yr (44658 d)
- Aphelion
- 3.5124 AU (525.45 Gm )
- Perihelion
- 2.93357 AU (438.856 Gm)
- Semi major axis
- 3.22298 AU (482.151 Gm)
- Orbital period sidereal
- 5.79 yr (2113.4 d )
- Mean anomaly
- 350.739 °
- Mean motion
- 0° 10 13.224 / day
- Inclination
- 12.558°
- Longitude of ascending node
- 125.102°
- Argument of perihelion
- 142.930°
- Dimensions
- 120.58 ± 2.7 km , 147.2×126.6 km, 123.41 ± 6.30 km
- Mass
- (9.18 ± 0.80) × 10 kg
via Wikipedia infobox
Wikidata facts
- Instance of
- asteroid
- Named after
- Myrrha
- Followed by
- 382 Dodona
- Follows
- 380 Fiducia
- Parent body
- Sun
- Diameter
- 127.639
- Orbital period
- 2124.367834340938
Show 19 more facts
- discoverer or inventor
- Auguste Charlois
- site of astronomical discovery
- Nice Observatory
- provisional designation
- A894 AC
- time of discovery or invention
- 1894-01-10
- asteroid spectral type
- C-type asteroid
- orbital inclination
- 12.6099828639309
- Commons category
- 381 Myrrha
- albedo
- 0.064
- rotation period
- 6.572
- absolute magnitude
- 8.38
- orbital eccentricity
- 0.08789247842360084
- semi-major axis of an orbit
- 3.234105578029831
- periapsis
- 2.949852023293197
- apoapsis
- 3.518359132766465
- longitude of ascending node
- 124.7153787120321
- argument of periapsis
- 148.2581829555188
- mean anomaly
- 203.924056054258
- time of periapsis
- 2461921.5075417575
- epoch
- November 21, 2025
Sources (2)
via Wikidata · CC0
~1 min read
Encyclopedic overview
381 Myrrha is a main-belt asteroid that was discovered by the French astronomer Auguste Charlois on January 10, 1894, in Nice. It has been classified as a C-type asteroid and is most likely composed of carbonaceous material.
Photometric observations of this asteroid at the Oakley Observatory in Terre Haute, Indiana during 2006 gave a light curve with a period of 6.572 ± 0.002 hours and a brightness variation of 0.34 ± 0.05 in magnitude.
Excerpted from Wikipedia’s “381 Myrrha” article, available under the CC BY-SA 4.0 licence.