Linus (moon)

{{Short description|Asteroid moon that orbits 22 Kalliope}}

{{Infobox planet | bgcolour=#A0FFA0 | minorplanet=yes

| name=Linus

| image = 22-Kalliope-Linus.jpg

| caption = Kalliope and satellite Linus as seen by the W.M. Keck II telescope in 2010

| pronounced={{IPAc-en|ˈ|l|aɪ|n|ə|s}}

| adjectives=Linian {{IPAc-en|ˈ|l|ɪ|n|i|ə|n}}"linia" = 'of Linus' in Banier (1793) The mythology and fables of the ancients, explain'd from history, v. 1; also in Charles Frederick Partington (1838) The British Cyclopædia of Biography

| discovery_ref =

| discoverer=Jean-Luc Margot and Michael E. Brown

| discovered=August 29, 2001

| mpc_name = Kalliope I

| alt_names=S/2001 (22) 1

| named_after = Linus

| mp_category=Main belt

| semimajor= 1063 ± 23 km (1040-1086)

1099 ± 11 km (1088-1110)

| eccentricity=<0.015

<0.005

| period=3.596 ± 0.040 d (3.556-3.636)

3.590 ± 0.001 d[http://astro.berkeley.edu/~fmarchis/Science/Asteroids/Kalliope.html synthesis of several observations] {{webarchive|url=https://web.archive.org/web/20060829010621/http://astro.berkeley.edu/~fmarchis/Science/Asteroids/Kalliope.html |date=2006-08-29 }} including recent ones with the VLT 8m telescope. (3.589-3.591)

| avg_speed=21.5 m/s

| inclination= ~0°
(undetectable with respect to Kalliope equator)

| satellite_of = 22 Kalliope

| dimensions=28 ± 2 km

| mass=~6{{e|16}} kg (estimate)

~4{{e|16}} kg (estimate)

| density = 3.4 g/cm3 (assumed)

| escape_velocity=~20 m/s (estimate)

| rotation = unknown, probably synchronousBased on a rough tidal locking timescale of several tens of My.

| axial_tilt = unknown, zero expected

| temp_name1 = Kelvin

| mean_temp_1 = ~161

| max_temp_1 = 240

| temp_name2 = Celsius

| mean_temp_2 = ~ -113

| max_temp_2 = −32°

| abs_magnitude=9.7

}}

Linus, formal designation (22) Kalliope I, is an asteroid moon that orbits the large M-type asteroid 22 Kalliope. It was discovered on August 29, 2001, by astronomers Jean-Luc Margot and Michael E. Brown with the Keck telescope, in Hawaii. Another team also detected the moon with the Canada-France-Hawaii Telescope on September 2, 2001. Both telescopes are on Mauna Kea. It received the provisional designation S/2001 (22) 1, until it was named. The naming proposal appeared in the discovery paper and was approved by the International Astronomical Union in July 2003. Although the naming proposal referred to the mythological Linus, son of the muse Calliope and the inventor of melody and rhythm, the name was also meant to honor Linus Torvalds, inventor of the Linux operating system kernel, and Linus van Pelt, a character in the Peanuts comic strip.{{cite web|url=http://www2.ess.ucla.edu/~jlm/research/MBAs/Kalliope/index.html|author=Margot, Jean-Luc|title=Adaptive Optics Observations of Kalliope-Linus|date=2004|work=UCLA|accessdate=2013-08-30}}

With an estimated {{nowrap|28 ± 2 km}} (17 ± 1 mi) diameter, Linus is very large compared to most asteroid moons, and would be a sizable asteroid by itself. The only known larger moons in the main belt are the smaller components of the double asteroids 617 Patroclus and 90 Antiope.

It has been estimated that Linus' orbit precesses at quite a rapid rate, making one cycle in several years. This is attributed primarily to the non-spherical shape of Kalliope. Linus's brightness has varied appreciably between observations, which may indicate that its shape is elongated.

Linus may have formed out of impact ejecta from a collision with Kalliope, or a fragment captured after disruption of a parent asteroid (a proto-Kalliope).

References

{{reflist

| refs =

{{cite web

|date=September 3, 2001

|title=IAUC 7703: S/2001 (22) 1; 2001ed

|publisher=IAU Central Bureau for Astronomical Telegrams

|url=http://www.cbat.eps.harvard.edu/iauc/07700/07703.html

|accessdate=2012-07-18}}

{{cite journal | author= J.L. Margot & M.E. Brown| title= A Low-Density M-type Asteroid in the Main Belt| journal= Science| date= 2003| volume= 300| pages= 1939–42| doi= 10.1126/science.1085844| pmid= 12817147 | issue= 5627| bibcode=2003Sci...300.1939M}}

{{cite web

|date=August 8, 2003

|title=IAUC 8177: Sats of (22); Sats of Jupiter, Saturn, Uranus

|publisher=IAU Central Bureau for Astronomical Telegrams

|url=http://www.cbat.eps.harvard.edu/iauc/08100/08177.html

|accessdate=2012-07-18}}

{{cite journal | author= F. Marchis| title= A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope| journal= Icarus| date= 2003| volume= 165 | issue= 1| pages= 112| bibcode=2003Icar..165..112M| doi= 10.1016/S0019-1035(03)00195-7 | display-authors= 1 | last2= Descamps | first2= P. | last3= Hestroffer | first3= D. | last4= Berthier | first4= J. | last5= Vachier | first5= F. | last6= Boccaletti | first6= A. | last7= De Pater | first7= I. | last8= Gavel | first8= D.}}

{{cite journal|last=Descamps|first=P.|title=New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses|date=2008|journal=Icarus|volume=196|issue=2| pages=578–600|bibcode=2008Icar..196..578D|doi=10.1016/j.icarus.2008.03.014| arxiv=0710.1471|author2=Marchis, F.|last3=Pollock|first3=J.|display-authors=2|last4=Berthier|first4=J|last5=Vachier|first5=F|last6=Birlan|first6=M|last7=Kaasalainen|first7=M|last8=Harris|first8=A|last9=Wong|first9=M }}

}}