Notable Asteroids, Part 2 Codexery

1866 Sisyphus

Largest Apollo-group asteroid, binary, and near-Earth object.

1866 Sisyphus

1866 Sisyphus is a binary, stony asteroid that orbits near Earth and is the largest known member of the Apollo group, with a diameter of about 7 kilometers. Swiss astronomer Paul Wild discovered it on December 5, 1972, at the Zimmerwald Observatory near Bern, Switzerland. Its name comes from the Greek mythological king Sisyphus. This S-type asteroid, made of rocky silicates, travels around the Sun at distances ranging from 0.9 to 2.9 AU, completing one orbit every 2 years and 7 months (952 days). Its orbit is highly elongated, with an eccentricity of 0.54, and steeply tilted at 41° relative to the ecliptic. As an Apollo asteroid, its closest possible approach to Earth is 0.1037 AU (about 15.5 million kilometers, or 40.4 lunar distances). On November 24, 2071, it will pass 0.11581 AU (17.3 million kilometers) from Earth, reaching an apparent magnitude of roughly 9.3 on November 26. When discovered in 1972, it peaked at magnitude 9.0 on November 25, making it one of the brightest near-Earth asteroids. In the SMASS classification, Sisyphus is a common stony S-type. Radar observations from the Arecibo Observatory in 1985, at a distance of 0.25 AU, measured its radar cross-section at 8 square kilometers. These observations also detected a small moon orbiting the asteroid, though its existence wasn't reported until December 2007. Robert Stephens confirmed that it is a suspected binary, and Brian Warner added additional weight to this conclusion.

Quick Facts

Minorplanet
yes
Background
#FFC2E0
Discovered
5 December 1972
Discoverer
P. Wild
Discovery Site
Zimmerwald Obs.
Mpc Name
(1866) Sisyphus
Pronounced
ˈ · s · ɪ · s · ᵻ · f · ə · s
Adjectives
Sysiphean s · ɪ · s · ᵻ · ˈ · f · iː · ən, Sisyphian s · ɪ · ˈ · s · ɪ · f · i · ə · n
Named After
Σίσυφος Sīsyphos (Greek mythology)
Mp Category
Apollo · NEO · Mars-crosser
Epoch
4 September 2017 (JD 2458000.5)
Uncertainty
0

Facts from the source article.

Lore & Background

1866 Sisyphus orbits the Sun in the inner main-belt at a distance of 0.9–2.9 AU once every 2 years and 7 months (952 days). Its orbit has an eccentricity of 0.54 and an inclination of 41° with respect to the ecliptic. The Apollo asteroid has an Earth minimum orbit intersection distance of 0.1037 AU (15,500,000 km), corresponding to 40.4 lunar distances. It will pass 0.11581 AU (17,325,000 km) from Earth on 24 November 2071, and will peak at roughly apparent magnitude 9.3 on 26 November 2071. When discovered it peaked at magnitude 9.0 on 25 November 1972. It is one of the brightest near-Earth asteroids. In the SMASS classification, Sisyphus is a common stony S-type asteroid. In 1985, it was detected with radar from the Arecibo Observatory at a distance of 0.25 AU, with a measured radar cross-section of 8 square kilometers. During the radar observations, a small minor-planet moon was detected around Sisyphus, although its existence was not reported until December 2007. Robert Stephens confirmed that it is a suspected binary, and Brian Warner added additional weight to this conclusion, giving hours as the satellite's orbital period, longer than the 25 hours previously reported by Stephens.

Reader's Guide

1866 Sisyphus is notable as the largest member of the Apollo group of near-Earth asteroids, with a diameter comparable to the Chicxulub impactor. Its binary nature, discovered via radar in 1985 but only reported in 2007, adds to its scientific interest. The asteroid's orbit brings it relatively close to Earth, with a minimum orbit intersection distance of 0.1037 AU (15.5 million km), and it will make a notable approach in November 2071, reaching apparent magnitude 9.3. As one of the brightest near-Earth asteroids, it has been studied for its physical characteristics, including its stony S-type composition. Its naming after the mythological figure Sisyphus reflects the perpetual motion of its orbit. The asteroid's size and Earth-crossing status make it a significant object for understanding potential impact hazards, though the article does not classify it as an immediate threat. The discovery of its satellite and the subsequent refinement of the moon's orbital period highlight ongoing research into binary asteroid systems.

Did You Know?

Frequently Asked Questions

What is 1866 Sisyphus?

1866 Sisyphus is a stony, binary near-Earth asteroid roughly 7 kilometers across, making it the largest confirmed member of the Apollo group. It follows a highly stretched orbit that carries it between 0.9 and 2.9 AU from the Sun.

Who discovered 1866 Sisyphus and where?

Swiss astronomer Paul Wild spotted it on 5 December 1972 from the Zimmerwald Observatory just outside Bern, Switzerland. It carried the provisional designation 1972 XA before receiving its permanent number and name.

Why is the asteroid named Sisyphus?

The name honors Sisyphus, the king from Greek mythology condemned to roll a boulder uphill for eternity. The fitting choice mirrors the asteroid's long, eccentric orbital path that repeatedly swings it close to Earth before flinging it far out again.

What makes 1866 Sisyphus stand out among near-Earth asteroids?

It holds the record as the biggest known Apollo-group object and is one of the few confirmed binary near-Earth asteroids. Its S-type composition means it is built mostly from rocky silicate material rather than metal or carbon.

How long does 1866 Sisyphus take to orbit the Sun, and what is its orbit like?

One full trip around the Sun takes about 952 days—roughly two years and seven months. The orbit is notably elongated with an eccentricity of 0.54 and tilted 41 degrees relative to the ecliptic plane.

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