1I/'Oumuamua 1I/'Oumuamua Fr.: 1I/'Oumuamua The first known → interstellar object coming from beyond → Solar System. Detected on October 19, 2017 by the → Pan-STARRS sky survey, it was initially classified as an interstellar → asteroid. ‘Oumuamua has a strongly → hyperbolic orbit
(→ eccentricity
1.191 ± 0.007), with a very high average velocity
with respect to the Sun (v∞ =
26.32 km s-1), indicating that it likely originated from beyond our
Solar System. Its → inclination
with respect to the → ecliptic is
123°. ‘Oumuamua would be approximately 160 m in diameter. When first detected, ‘Oumuamua was 0.2 → astronomical units (au) from the Earth (30 × 106 km). Initially it was classified to be a → comet and was designated C/2017 U1. But further observations revealed no hint of → cometary activity. The object was therefore reclassified as an asteroid with designation A/2017 U1. According to orbit calculations, ‘Oumuamua Pulled by the Sun’s gravity, the object made a U turn below the ecliptic, passing under Earth’s orbit on October 14 at a distance of about 24 million km, that is about 60 times the distance to the Moon. It has now risen above the plane of the planets and is travelling at 44 km s-1 with respect to the Sun. In 2197 it will be 1,000 au from the Sun. Recent → outgassing activity observed toward this object suggests that ‘Oumuamua is most likely an interstellar comet and not an asteroid (Michelli et al., 2018, Nature 27 June). See also: The name ‘Oumuamua approved by the IAU was submitted by the team at
the Pan-STARRS telescope who discovered the object. It is a
Hawaiian construct combining ‘ou “to reach out” and mua
“first” or “in advance of;” the second mua is for emphasis. |