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1551 Argelander

Main-belt asteroid


Summary

Main-belt asteroid

FieldValue
minorplanetyes
name1551 Argelander
background#D6D6D6
imageFile:001551-asteroid shape model (1551) Argelander.png
captionShape model of Argelander from its lightcurve
discovery_ref
discovererY. Väisälä
discovery_siteTurku Observatory
discovered24 February 1938
mpc_name(1551) Argelander
alt_names1930 BL
1940 XD
1957 KR
1962 XP
named_afterFriedrich Argelander
(German astronomer)
mp_categorymain-belt(inner)
background
orbit_ref
epoch27 April 2019 (JD 2458600.5)
uncertainty0
observation_arc88.76 yr (32,418 d)
aphelion2.5539 AU
perihelion2.2350 AU
semimajor2.3944 AU
eccentricity0.0666
period3.71 yr (1,353 d)
mean_anomaly147.41°
mean_motion/ day
inclination3.7615°
asc_node107.23°
arg_peri233.60°
mean_diameter
rotation
albedo
spectral_typeS (assumed)
abs_magnitude12.10
12.20

1940 XD 1957 KR 1962 XP (German astronomer) background

12.20

1551 Argelander (provisional designation ****) is a background asteroid from the inner regions of the asteroid belt, approximately 10 km in diameter. It was discovered on 24 February 1938, by Finnish astronomer Yrjö Väisälä at the Turku Observatory in southwest Finland. The likely S-type asteroid has a rotation period of 4.1 hours. It was named after German astronomer Friedrich Argelander.

Orbit and classification

Argelander is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner main-belt at a distance of 2.2–2.6 AU once every 3 years and 9 months (1,353 days; semi-major axis of 2.39 AU). Its orbit has an eccentricity of 0.07 and an inclination of 4° with respect to the ecliptic. The body's observation arc begins with its first observation as at Heidelberg Observatory in January 1930, or 8 years prior to its official discovery observation at Turku.

Naming

This minor planet was named after Friedrich Wilhelm Argelander (1799–1875), author of the Bonner Durchmusterung and 19th-century head of the ancient observatory at Turku and Bonn . The official was published by the Minor Planet Center on 30 January 1964 (M.P.C. 2278). The lunar crater Argelander is also named after him.

Physical characteristics

Argelander is an assumed S-type asteroid.

Rotation period and poles

In August 2017, a rotational lightcurve of Argelander was obtained from photometric observations at the Chilean Cerro Tololo Inter-American Observatory using the SARA South Telescope. Lightcurve analysis gave a rotation period of hours and a brightness variation of 0.48 magnitude (). In January 2012, astronomers at the Palomar Transient Factory had also determined a period of with an amplitude of 0.41 magnitude ().

A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016. It gave a concurring period of hours, as well as two spin axes at (3.0°, −81.0°) and (183.0°, −72.0°) in ecliptic coordinates (λ, β).

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Argelander measures between 9.2 and 11.0 kilometers in diameter and its surface has an albedo between 0.19 and 0.30. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 9.60 kilometers based on an absolute magnitude of 12.45.

References

Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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