19738 Calinger

{{Short description|Main-belt asteroid}}

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

{{Infobox planet

| minorplanet = yes

| name = 19738 Calinger

| background = #D6D6D6

| image =

| image_size =

| caption =

| discovery_ref =

| discovered = 4 January 2000

| discoverer = LINEAR

| discovery_site = Lincoln Lab's ETS

| mpc_name = (19738) Calinger

| alt_names = {{nowrap|{{mp|2000 AS|97}}{{·}}{{mp|1991 RZ|36}}}}

| named_after = Manetta Calinger
{{small|(DCYSC mentor)}}

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

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 26.88 yr (9,819 days)

| aphelion = 2.7043 AU

| perihelion = 1.8606 AU

| semimajor = 2.2824 AU

| eccentricity = 0.1848

| period = 3.45 yr (1,260 days)

| mean_anomaly = 165.65°

| mean_motion = {{Deg2DMS|0.2858|sup=ms}} / day

| inclination = 7.7356°

| asc_node = 90.753°

| arg_peri = 280.16°

| dimensions = {{val|3.272|0.082}}

| rotation =

| albedo = {{val|0.314|0.056}}

| spectral_type =

| abs_magnitude = 14.1

}}

19738 Calinger (provisional designation {{mp|2000 AS|97}}) is a background asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter.

It was discovered on 4 January 2000, by members of the Lincoln Near-Earth Asteroid Research team at Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico, and named after DCYSC-mentor Manetta Calinger.

Classification and orbit

Calinger is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,260 days). Its orbit has an eccentricity of 0.18 and an inclination of 8° with respect to the ecliptic.

The body's observation arc begins almost 10 years prior to its official discovery observation, with a precovery from the Digitized Sky Survey taken at Palomar Observatory in May 1990.

Physical characteristics

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Calinger measures 3.272 kilometers in diameter and its surface has a high albedo of 0.314. It has an absolute magnitude of 14.1.

= Lightcurves =

As of 2017, Calinger's rotation period and shape remain unknown.

Naming

This minor planet was named after Manetta Calinger who mentored a finalist in the 2003 Discovery Channel Youth Science Challenge, DCYSC. The approved naming citation was published by the Minor Planet Center on 10 October 2003 ({{small|M.P.C. 49772}}).

References

{{reflist|30em|refs=

{{cite web

|type = 2017-03-31 last obs.

|title = JPL Small-Body Database Browser: 19738 Calinger (2000 AS97)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2019738

|publisher = Jet Propulsion Laboratory

|access-date = 26 June 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (19738) Calinger, Addendum to Fifth Edition: 2003–2005

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 142

|date = 2006

|isbn = 978-3-540-34361-5

|doi = 10.1007/978-3-540-34361-5_1596 |chapter = (19738) Calinger [2.28, 0.19, 7.7] }}

{{cite web

|title = 19738 Calinger (2000 AS97)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=19738

|access-date = 9 March 2017}}

{{cite web

|title = MPC/MPO/MPS Archive

|work = Minor Planet Center

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

|access-date = 9 March 2017}}

{{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 = J. |last6 = Dailey

|first7 = P. R. M. |last7 = Eisenhardt

|first8 = R. S. |last8 = McMillan

|first9 = T. B. |last9 = Spahr

|first10 = M. F. |last10 = Skrutskie

|first11 = D. |last11 = Tholen

|first12 = R. G. |last12 = Walker

|first13 = E. L. |last13 = Wright

|first14 = E. |last14 = DeBaun

|first15 = D. |last15 = Elsbury

|first16 = T. IV |last16 = Gautier

|first17 = S. |last17 = Gomillion

|first18 = A. |last18 = Wilkins

|date = November 2011

|title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M

|journal = The Astrophysical Journal

|volume = 741

|issue = 2

|page = 20

|bibcode = 2011ApJ...741...68M

|doi = 10.1088/0004-637X/741/2/68

|arxiv = 1109.4096

|access-date= 9 March 2017}}

{{cite web

|title = LCDB Data for (19738) Calinger

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=19738%7CCalinger

|access-date = 26 June 2017}}

}}