1551 Argelander

{{Short description|Main-belt asteroid}}

{{Use dmy dates|date=December 2018}}

{{Infobox planet

| minorplanet = yes

| name = 1551 Argelander

| background = #D6D6D6

| image = File:001551-asteroid shape model (1551) Argelander.png

| image_scale =

| caption = Shape model of Argelander from its lightcurve

| discovery_ref =

| discoverer = Y. Väisälä

| discovery_site = Turku Obs.

| discovered = 24 February 1938

| mpc_name = (1551) Argelander

| alt_names = {{mp|1938 DC|1}}{{·}}1930 BL
1940 XD{{·}}{{mp|1951 XG|1}}
{{mp|1953 GD|1}}{{·}}1957 KR
1962 XP

| pronounced =

| named_after = {{nowrap|Friedrich Argelander}}
{{small|(German astronomer)}}

| mp_category = main-belt{{·}}{{small|(inner)}}
background

| orbit_ref =

| epoch = 27 April 2019 (JD 2458600.5)

| uncertainty = 0

| observation_arc = 88.76 yr (32,418 d)

| aphelion = 2.5539 AU

| perihelion = 2.2350 AU

| semimajor = 2.3944 AU

| eccentricity = 0.0666

| period = 3.71 yr (1,353 d)

| mean_anomaly = 147.41°

| mean_motion = {{Deg2DMS|0.2660|sup=ms}} / day

| inclination = 3.7615°

| asc_node = 107.23°

| arg_peri = 233.60°

| mean_diameter = {{val|9.19|0.27|ul=km}}
{{val|10.238|0.122|u=km}}
{{val|10.50|0.50|u=km}}
{{val|11.016|0.073|u=km}}

| rotation = {{val|4.063|0.006|ul=h}}

| albedo = {{val|0.1940}}
{{val|0.217}}
{{val|0.222}}
{{val|0.302}}

| spectral_type = S {{small|(assumed)}}

| abs_magnitude = 12.10
12.20

}}

1551 Argelander, provisional designation {{mp|1938 DC|1}}, is a background asteroid from the inner regions of the asteroid belt, approximately {{convert|10|km|mi|abbr=off|sigfig=2|sp=us}} 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 {{mp|1930 BL}} 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 famous Bonner Durchmusterung and 19th-century head of the ancient observatory at Turku and Bonn {{Obscode|520}}. The official {{MoMP|1551|naming citation}} was published by the Minor Planet Center on 30 January 1964 ({{small|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 {{val|4.063|0.006}} hours and a brightness variation of 0.48 magnitude ({{small|U=2+}}). In January 2012, astronomers at the Palomar Transient Factory had also determined a period of {{val|4.061|0.0023}} with an amplitude of 0.41 magnitude ({{small|U=2}}).

A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016. It gave a concurring period of {{val|4.058350|0.000001}} 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

{{reflist|30em|refs=

{{cite web

|type = 2018-10-20 last obs.

|title = JPL Small-Body Database Browser: 1551 Argelander (1938 DC1)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001551

|publisher = Jet Propulsion Laboratory

|accessdate = 11 December 2018}}

{{cite book

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|date = 2007

|isbn = 978-3-540-00238-3

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|chapter-url = https://cds.cern.ch/record/1339661

}}

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{{cite web

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|publisher = AstDyS-2, Asteroids – Dynamic Site

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|accessdate = 10 December 2018}}

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|work = Small Bodies Data Ferret

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|accessdate = 11 December 2018}}

{{cite web

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|publisher = Asteroid Lightcurve Database (LCDB)

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}}