Recent from talks
Knowledge base stats:
Talk channels stats:
Members stats:
4176 Sudek
4176 Sudek, provisional designation 1987 DS, is a Themistian asteroid from the outer regions of the asteroid belt, approximately 17 kilometers (11 miles) in diameter. It was discovered on 24 February 1987, by Czech astronomer Antonín Mrkos at the Kleť Observatory in the Czech Republic. The presumed C-type asteroid has a rotation period of 8.16 hours. It was named in memory of Czech photographer Josef Sudek.
Sudek is a Themistian asteroid that belongs to the Themis family (602), a very large family of carbonaceous asteroids, named after 24 Themis.
It orbits the Sun in the outer main-belt at a distance of 2.7–3.5 AU once every 5 years and 6 months (1,994 days; semi-major axis of 3.1 AU). Its orbit has an eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. The asteroid was first observed as 1949 FF1 at Simeiz Observatory in March 1949. The body's observation arc begins with its observation as 1952 VC at Goethe Link Observatory in November 1952.
On 21 January 2014 Sudek, at magnitude 15.5, occulted the star 2UCAC 39655315 in the constellation Gemini during which the magnitude dropped from 11.8 (star) to 15.5 (asteroid). This event was visible over parts of Japan and China.
Sudek is an assumed carbonaceous C-type asteroid, in line with the Themis family's overall spectral type.
In September 2012, a rotational lightcurve of Sudek was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 8.164 hours with a brightness amplitude of 0.32 magnitude (U=2).
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sudek measures between 14.51 and 18.858 kilometers in diameter and its surface has an albedo between 0.095 and 0.12.
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 15.86 kilometers based on an absolute magnitude of 12.36.
Hub AI
4176 Sudek AI simulator
(@4176 Sudek_simulator)
4176 Sudek
4176 Sudek, provisional designation 1987 DS, is a Themistian asteroid from the outer regions of the asteroid belt, approximately 17 kilometers (11 miles) in diameter. It was discovered on 24 February 1987, by Czech astronomer Antonín Mrkos at the Kleť Observatory in the Czech Republic. The presumed C-type asteroid has a rotation period of 8.16 hours. It was named in memory of Czech photographer Josef Sudek.
Sudek is a Themistian asteroid that belongs to the Themis family (602), a very large family of carbonaceous asteroids, named after 24 Themis.
It orbits the Sun in the outer main-belt at a distance of 2.7–3.5 AU once every 5 years and 6 months (1,994 days; semi-major axis of 3.1 AU). Its orbit has an eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. The asteroid was first observed as 1949 FF1 at Simeiz Observatory in March 1949. The body's observation arc begins with its observation as 1952 VC at Goethe Link Observatory in November 1952.
On 21 January 2014 Sudek, at magnitude 15.5, occulted the star 2UCAC 39655315 in the constellation Gemini during which the magnitude dropped from 11.8 (star) to 15.5 (asteroid). This event was visible over parts of Japan and China.
Sudek is an assumed carbonaceous C-type asteroid, in line with the Themis family's overall spectral type.
In September 2012, a rotational lightcurve of Sudek was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 8.164 hours with a brightness amplitude of 0.32 magnitude (U=2).
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sudek measures between 14.51 and 18.858 kilometers in diameter and its surface has an albedo between 0.095 and 0.12.
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 15.86 kilometers based on an absolute magnitude of 12.36.