3905 Doppler, provisional designation , is a stony
asteroid
An asteroid is a minor planet of the inner Solar System. Sizes and shapes of asteroids vary significantly, ranging from 1-meter rocks to a dwarf planet almost 1000 km in diameter; they are rocky, metallic or icy bodies with no atmosphere.
...
and
binary system from the middle region of the
asteroid belt, approximately 8 kilometers in diameter.
The asteroid was discovered on 28 August 1984, by Czech astronomer
Antonín Mrkos at
Kleť Observatory
Kleť Observatory ( cz, Hvězdárna Kleť; obs. code: 046) is an astronomical observatory in the Czech Republic. It is situated in South Bohemia, south of the summit of Mount Kleť, near the town of České Budějovice. Constructed in 1957, t ...
and named after physicist
Christian Doppler.
Orbit and characterization
''Doppler'' orbits the Sun in the
central
Central is an adjective usually referring to being in the center of some place or (mathematical) object.
Central may also refer to:
Directions and generalised locations
* Central Africa, a region in the centre of Africa continent, also known as ...
main-belt at a distance of 1.9–3.2
AU once every 4 years and 1 month (1,496 days). Its orbit has an
eccentricity of 0.26 and an
inclination of 14
° with respect to the
ecliptic.
It has been characterized as a common
S-type asteroid.
A
minor-planet moon orbiting ''Doppler'' every 50.8 hours (or 2 days, 2 hours, and 48 minutes) was found orbiting the asteroid in 2013. This is fairly long
orbital period for a moon of an asteroid of this size.
The satellite's orbital period is identical to the primary's
rotation period
The rotation period of a celestial object (e.g., star, gas giant, planet, moon, asteroid) may refer to its sidereal rotation period, i.e. the time that the object takes to complete a single revolution around its axis of rotation relative to the ...
(F-type binary).
According to the survey carried out by NASA's
Wide-field Infrared Survey Explorer with its subsequent
NEOWISE mission, ''Doppler'' measures 8.021 kilometers in diameter and its surface has an
albedo of 0.228,
while the ''Collaborative Asteroid Lightcurve Link'' assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.97 kilometers with an
absolute magnitude of 12.6.
Naming
This
minor planet was named after
Christian Doppler (1803–1853), Austrian physicist in Vienna and well known for the
Doppler effect
The Doppler effect or Doppler shift (or simply Doppler, when in context) is the change in frequency of a wave in relation to an observer who is moving relative to the wave source. It is named after the Austrian physicist Christian Doppler, who d ...
, which he first described in 1842, in his book "Ueber das farbige Licht der Doppelsterne". The naming was proposed by
Jana Tichá and M. Šolc.
The approved naming citation was published by the
Minor Planet Center
The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU). Founded in 1947, it operates at the Smithsonian Astrophysical Observatory.
Function
...
on 28 August 1996 ().
References
External links
Asteroids with Satellites Robert Johnston, johnstonsarchive.net
Asteroid Lightcurve Database (LCDB) query form
)
Dictionary of Minor Planet Names Google books
– Observatoire de Genève, Raoul Behrend
– Minor Planet Center
*
*
{{DEFAULTSORT:Doppler
003905
Discoveries by Antonín Mrkos
Named minor planets
003905
19840828