2308 Schilt

{{Short description|Minor planet}}

{{Use dmy dates|date=October 2019}}

{{Infobox planet

| minorplanet = yes

| name = 2308 Schilt

| background = #D6D6D6

| image =

| image_size =

| caption =

| discovery_ref =  

| discovered = 6 May 1967

| discoverer = C. U. Cesco
A. R. Klemola

| discovery_site = El Leoncito
{{nowrap|{{small|(Yale–Columbia Southern Station)}}}}

| mpc_name = (2308) Schilt

| alt_names = 1967 JM{{·}}1926 GP
1930 DR{{·}}{{mp|1972 TX|7}}
{{mp|1976 UH|12}}{{·}}1980 VF
1981 YM

| named_after = Jan Schilt {{small|(astronomer)}}

| mp_category = main-belt{{·}}Eunomia

| orbit_ref =  

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 82.71 yr (30,210 days)

| aphelion = 2.9873 AU

| perihelion = 2.1114 AU

| semimajor = 2.5494 AU

| eccentricity = 0.1718

| period = 4.07 yr (1,487 days)

| mean_anomaly = 117.70°

| mean_motion = {{Deg2DMS|0.2421|sup=ms}} / day

| inclination = 14.176°

| asc_node = 34.265°

| arg_peri = 233.60°

| dimensions = {{val|13.79|0.57}} km
17.51 km {{small|(derived)}}
{{val|17.54|0.8}} km {{small|(IRAS:18)}}
{{val|17.626|0.220}} km
{{val|17.719|0.098}} km

| rotation = {{val|9.759|0.002}} h
{{val|9.767|0.005}} h{{efn|name=lcdb-Mazzone}}

| albedo = 0.1001 {{small|(derived)}}
{{val|0.1088|0.0335}}
{{val|0.1094|0.011}} {{small|(IRAS:18)}}
{{val|0.177|0.024}}

| spectral_type = SMASS = S{{·}}S

| abs_magnitude = 11.8{{·}}11.9

}}

2308 Schilt, provisional designation {{mp|1967 JM}}, is a stony Eunomia asteroid from the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 6 May 1967, by Argentine astronomer Carlos Cesco together with American astronomer Arnold Klemola at the Yale–Columbia Southern Station at Leoncito Astronomical Complex in Argentina.

Orbit and classification

Schilt is a member of the Eunomia family, a large group of stony asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in the central main-belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,487 days). Its orbit has an eccentricity of 0.17 and an inclination of 14° with respect to the ecliptic. The asteroids observation arc begins with its discovery in 1967. However, the first (unused) precovery was already taken at Heidelberg Observatory in 1921.

Physical characteristics

In the SMASS taxonomy, Schilt has been characterized as a common S-type asteroid.

= Rotation period =

A rotational lightcurve was obtained based on photometric observations at the Australian Oakley Southern Sky Observatory in August 2012. The lightcurve showed a period of {{val|9.759|0.002}} hours with a brightness amplitude of 0.44 in magnitude ({{small|1=U=3}}). A previous observation by Argentine astronomer Salvador Mazzone at the Observatorio Astronómico Salvador gave a similar period of {{val|9.767|0.005}} with an amplitude of 0.42 in magnitude ({{small|1=U=3-}}).{{efn|name=lcdb-Mazzone}}

= Diameter and albedo =

According to the surveys carried out by the Infrared Astronomical Satellite (IRAS) and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 13.8 and 17.7 kilometers in diameter and its surface has an albedo in the range of 0.10–0.17. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.10 and a diameter of 17.5 kilometers.

Naming

This minor planet was named after Dutch–American astronomer Jan Schilt (1894–1982), one of the founders of the discovering Columbia–Yale Southern Station in the early 1960s, for which he collaborated with local astronomer and with Yale's Dirk Brouwer, after whom the minor planet 1746 Brouwer is named. At Columbia University, Schilt's research included the dynamics and structure of galaxies, and improvements in measuring the brightness of stars. The official naming citation was published by the Minor Planet Center on 11 December 1981 ({{small|M.P.C. 6531}}).

Notes

{{notelist|refs=

{{efn|name=lcdb-Mazzone|1=Mazzone (2012) web: rotation period {{val|9.767|0.005}} hours with a brightness amplitude of {{val|0.42}} mag and an LCDB quality code of U=3-. See [http://www.astrosurf.com/salvador/Fotometria.html at astrosurf]. Summary figures for (2308) Schilt at [http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2308%7CSchilt Collaborative Asteroid Lightcurve Link (CALL)]}}

}}

References

{{reflist|30em|refs=

{{cite web

|type = 2016-11-21 last obs.

|title = JPL Small-Body Database Browser: 2308 Schilt (1967 JM)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002308

|publisher = Jet Propulsion Laboratory

|accessdate = 12 June 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (2308) Schilt

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 188

|date = 2007

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

|doi = 10.1007/978-3-540-29925-7_2309 |chapter = (2308) Schilt }}

{{cite web

|title = 2308 Schilt (1967 JM)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=2308

|accessdate = 19 April 2016}}

{{cite web

|title = MPC/MPO/MPS Archive

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html

|accessdate = 18 May 2016}}

{{cite book

|year = 2014

|publisher = Springer Publishing

|pages = 1939–1940

|isbn = 978-0-387-31022-0

|doi = 10.1007/978-1-4419-9917-7_9396

|last1 = Milone

|first1 = Eugene F. |title = Biographical Encyclopedia of Astronomers

|chapter = Schilt, Jan

}}

{{cite web

|title = LCDB Data for (2308) Schilt

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2308%7CSchilt

|accessdate = 18 May 2016}}

{{cite journal

|display-authors = 6

|first1 = Joseph R. |last1 = Masiero

|first2 = A. K. |last2 = Mainzer

|first3 = T. |last3 = Grav

|first4 = J. M. |last4 = Bauer

|first5 = R. M. |last5 = Cutri

|first6 = C. |last6 = Nugent

|first7 = M. S. |last7 = Cabrera

|date = November 2012

|title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M

|journal = The Astrophysical Journal Letters

|volume = 759

|issue = 1

|page = 5

|bibcode = 2012ApJ...759L...8M

|doi = 10.1088/2041-8205/759/1/L8

|arxiv = 1209.5794

|access-date= 18 May 2016}}

{{cite journal

|display-authors = 6

|first1 = A. |last1 = Mainzer

|first2 = T. |last2 = Grav

|first3 = J. |last3 = Masiero

|first4 = E. |last4 = Hand

|first5 = J. |last5 = Bauer

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|first13 = C. |last13 = Maleszewski

|date = November 2011

|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M

|journal = The Astrophysical Journal

|volume = 741

|issue = 2

|page = 25

|bibcode = 2011ApJ...741...90M

|doi = 10.1088/0004-637X/741/2/90

|arxiv = 1109.6407

|access-date= 18 May 2016}}

{{Cite journal

|display-authors = 6

|first1 = Gary |last1 = Simpson

|first2 = Elena |last2 = Chong

|first3 = Michael |last3 = Gerhardt

|first4 = Sean |last4 = Gorsky

|first5 = Matthew |last5 = Klaasse

|first6 = Brian |last6 = Kodalen

|first7 = Faye |last7 = Li

|first8 = Luke |last8 = Mader

|first9 = Robert |last9 = Moore

|first10 = Rachel |last10 = Vinson

|first11 = Richard |last11 = Ditteon

|date = July 2013

|title = Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 August - October

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013MPBu...40..146S

|journal = The Minor Planet Bulletin

|volume = 40

|issue = 3

|pages = 146–151

|issn = 1052-8091

|bibcode = 2013MPBu...40..146S

|access-date= 18 May 2016}}

{{cite journal

|display-authors = 6

|first1 = Joseph R. |last1 = Masiero

|first2 = T. |last2 = Grav

|first3 = A. K. |last3 = Mainzer

|first4 = C. R. |last4 = Nugent

|first5 = J. M. |last5 = Bauer

|first6 = R. |last6 = Stevenson

|first7 = S. |last7 = Sonnett

|date = August 2014

|title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M

|journal = The Astrophysical Journal

|volume = 791

|issue = 2

|page = 11

|bibcode = 2014ApJ...791..121M

|doi = 10.1088/0004-637X/791/2/121

|arxiv = 1406.6645

|access-date= 7 December 2016}}

}}