1923 Osiris

{{Short description|Asteroid}}

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

{{Infobox planet

| minorplanet = yes

| name = 1923 Osiris

| background = #D6D6D6

| image =

| image_size =

| caption =

| discovery_ref =

| discovered = 24 September 1960

| discoverer = C. J. van Houten
I. van Houten G.
T. Gehrels

| discovery_site = Palomar Obs.

| mpc_name = (1923) Osiris

| alt_names = {{mp|4011 P-L}}{{·}}{{mp|1964 TO|2}}
1966 FR{{·}}1974 KN
1974 KP{{·}}1974 LE

| pronounced = {{IPAc-en|ə|ˈ|s|ai|r|ᵻ|s}}{{Cite encyclopedia |url=http://www.lexico.com/definition/Osiris |archive-url=https://web.archive.org/web/20200321100209/https://www.lexico.com/definition/osiris |url-status=dead |archive-date=21 March 2020 |title=Osiris |dictionary=Lexico UK English Dictionary |publisher=Oxford University Press}}

| named_after = {{nowrap|Osiris {{small|(Egyptian mythology)}}}}

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

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 62.70 yr (22,900 days)

| aphelion = 2.5900 AU

| perihelion = 2.2813 AU

| semimajor = 2.4356 AU

| eccentricity = 0.0634

| period = 3.80 yr (1,388 days)

| mean_anomaly = 269.38°

| mean_motion = {{Deg2DMS|0.2593|sup=ms}} / day

| inclination = 4.9580°

| asc_node = 353.07°

| arg_peri = 106.04°

| dimensions = 13.1 km
{{val|13.461|0.206}}

| rotation =

| albedo = {{val|0.031|0.006}}
0.0591 ± 0.008

| spectral_type = SMASS = C

| abs_magnitude = 13.6

}}

1923 Osiris, provisional designation {{mp|4011 P-L}}, is a dark asteroid from the inner regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 24 September 1960, by Ingrid and Cornelis Johannes van Houten at Leiden, on photographic plates taken by Tom Gehrels at Palomar Observatory in the United States. It was named after the Egyptian god Osiris.

Orbit and classification

Osiris orbits the Sun in the inner main-belt at a distance of 2.3–2.6 AU once every 3 years and 10 months (1,388 days). Its orbit has an eccentricity of 0.06 and an inclination of 5° with respect to the ecliptic. Due to a precovery taken at the discovering observatory in 1953, the body's observation arc is extended by 7 years prior to its official discovery observation.

= Palomar–Leiden survey =

The designation P–L stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis Johannes van Houten at Leiden Observatory. The trio are credited with several thousand asteroid discoveries.

Physical characteristics

In the SMASS classification, Osiris is a carbonaceous C-type asteroid.

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Osiris measures 13.461 kilometers in diameter and its surface has a low albedo of 0.031. As of 2017, no rotational lightcurve has been obtained.

Naming

This minor planet was named after Osiris, the Egyptian god of vegetation, of the waxing and waning Moon and of the annual flooding of the Nile. The official naming citation was published by the Minor Planet Center on 1 November 1979 ({{small|M.P.C. 5013}}).

References

{{reflist|30em|refs=

{{cite web

|type = 2016-08-18 last obs.

|title = JPL Small-Body Database Browser: 1923 Osiris (4011 P-L)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001923

|publisher = Jet Propulsion Laboratory

|accessdate = 14 June 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (1923) Osiris

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 154

|date = 2007

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

|doi = 10.1007/978-3-540-29925-7_1924 |chapter = (1923) Osiris }}

{{cite web

|title = 1923 Osiris (4011 P-L)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=1923

|accessdate = 14 June 2017}}

{{cite web

|title = MPC/MPO/MPS Archive

|work = Minor Planet Center

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

|accessdate = 14 June 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 = 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= 14 June 2017}}

{{cite web

|title = LCDB Data for (1923) Osiris

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1923%7COsiris

|accessdate = 14 June 2017}}

{{Citation | date = 1 Nov 1979 | title = New Names of Minor Planets | periodical = Minor Planet Circular | location = Cambridge, Mass | publisher = Minor Planet Center | issue = MPC 5013 | url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/1979/MPC_19791101.pdf | issn = 0736-6884 }}

}}