55576 Amycus

{{Use dmy dates|date=April 2020}}

{{Infobox planet

| minorplanet = yes

| background = #C7FF8F

| name = 55576 Amycus

| symbol = 24px (astrological)

| image = 55576 Amycus.tiff

| image_scale =

| caption = Orbital diagram (top view)

| discovery_ref =

| discoverer = NEAT

| discovery_site = Palomar

| discovered = 8 April 2002

| mpc_name = (55576) Amycus

| alt_names = {{mp|2002 GB|10}}

| pronounced = {{IPAc-en|ˈ|æ|m|ᵻ|k|ə|s}}Noah Webster (1884) A Practical Dictionary of the English Language

| adjectives = Amycian {{IPAc-en|@|ˈ|m|I|s|i|ə|n}}

| named_after = Amycus

| mp_category = Centaur

| orbit_ref =

| epoch = 13 January 2016 (JD 2457400.5)

| aphelion = {{Convert|35.019|AU|Tm|abbr=on|lk=on}} (Q)

| perihelion = {{Convert|15.178|AU|Tm|abbr=on}} (q)

| semimajor = {{Convert|25.098|AU|Tm|abbr=on}} (a)

| eccentricity = 0.39526 (e)

| period = 125.74 yr (45926.7 d)

| inclination = 13.352° (i)

| asc_node = 315.45° (Ω)

| mean_anomaly = 37.041° (M)

| arg_peri = 239.17° (ω)

| satellites =

| dimensions = {{Val|76.3|12.5|u=km}}

| mass =

| density =

| albedo = ~ 0.18

| spectral_type = {{Ubl

| B–V {{=}} {{val|1.111|0.034}}

| V–R {{=}} {{val|0.705|0.032}}

}}

| magnitude = ~ 20

| abs_magnitude = 7.8

| mean_motion = {{Deg2DMS|0.0078386|sup=ms}} / day (n)

| rotation = {{Convert|9.76|h|d|abbr=on|lk=on}}

| observation_arc = 7204 days (19.72 yr)

| uncertainty = 2

| jupiter_moid = {{Convert|9.92261|AU|Tm|abbr=on}}

| tisserand = 4.133

}}

55576 Amycus {{IPAc-en|ˈ|æ|m|ᵻ|k|ə|s}} is a centaur discovered on 8 April 2002 by the NEAT at Palomar.

The minor planet was named for Amycus, a male centaur in Greek mythology.

It came to perihelion in February 2003. Data from the Spitzer Space Telescope gave a diameter of {{Val|76.3|12.5|u=km}}.

A low probability asteroid occultation of star UCAC2 17967364 with an apparent magnitude of +13.8 was possible on 11 February 2009. Another such event involving a star with an apparent magnitude of +12.9 occurred on 10 April 2014 at about 10:46 Universal Time, visible for observers in the southwest US and western Mexico.

Near 3:4 resonance of Uranus

Amycus (2002 GB10) lies within 0.009 AU of the 3:4 resonance of Uranus and is estimated to have a long orbital half-life of about 11.1 Myr.{{Cite journal |last1=Showalter |first1=Mark R. |last2=Benecchi |first2=Susan D. |last3=Buie |first3=Marc W. |last4=Grundy |first4=William M. |last5=Keane |first5=James T. |last6=Lisse |first6=Carey M. |last7=Olkin |first7=Cathy B. |last8=Porter |first8=Simon B. |last9=Robbins |first9=Stuart J. |last10=Singer |first10=Kelsi N. |last11=Verbiscer |first11=Anne J. |last12=Weaver |first12=Harold A. |last13=Zangari |first13=Amanda M. |last14=Hamilton |first14=Douglas P. |last15=Kaufmann |first15=David E. |date=2021 |title=A statistical review of light curves and the prevalence of contact binaries in the Kuiper Belt |journal=Icarus |language=en |volume=356 |pages=114098 |doi=10.1016/j.icarus.2020.114098|s2cid=225284888 |doi-access=free |arxiv=2105.03543 |bibcode=2021Icar..35614098S }}

Image:AmycusAnim.gif) of Amycus.]]

See also

References

{{reflist

|refs=

{{cite web

|type= 2007-08-15 last obs

|title=JPL Small-Body Database Browser: 55576 Amycus (2002 GB10)

|url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=55576

|access-date=12 April 2016}}

{{Cite journal

|first1 = O. R. |last1 = Hainaut

|first2 = H. |last2 = Boehnhardt

|first3 = S. |last3 = Protopapa

|date = October 2012

|title = Colours of minor bodies in the outer solar system. II. A statistical analysis revisited

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012A&A...546A.115H

|journal = Astronomy and Astrophysics

|volume = 546

|page = 20

|bibcode = 2012A&A...546A.115H

|doi = 10.1051/0004-6361/201219566

|arxiv = 1209.1896

|s2cid = 54776793

|access-date= 26 September 2019}}

{{cite web

|author=Marc W. Buie

|author-link=Marc W. Buie

|type=2003-06-22 using 73 of 81 observations

|title=Orbit Fit and Astrometric record for 55576

|publisher=SwRI (Space Science Department)

|url=http://www.boulder.swri.edu/~buie/kbo/astrom/55576.html

|access-date=2009-02-28

|archive-url=https://web.archive.org/web/20110604032846/http://www.boulder.swri.edu/~buie/kbo/astrom/55576.html

|archive-date=4 June 2011

|url-status=dead

}}

{{cite arXiv

|title=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope

|author=John Stansberry

|author2=Will Grundy

|author3=Mike Brown

|author4=Dale Cruikshank

|author5=John Spencer

|author6=David Trilling

|author7=Jean-Luc Margot

|eprint=astro-ph/0702538

|date=2007-02-20}}

{{cite web

|date=22 August 2008

|title=List of Known Trans-Neptunian Objects

|publisher=Johnston's Archive

|author=Wm. Robert Johnston

|url=http://www.johnstonsarchive.net/astro/tnoslist.html

|access-date=2009-02-28

|archive-url= https://web.archive.org/web/20090213132019/http://johnstonsarchive.net/astro/tnoslist.html

|archive-date= 13 February 2009

|url-status= live}}

{{cite web

|title=AstDys (55576) Amycus Ephemerides

|publisher=Department of Mathematics, University of Pisa, Italy

|url=https://newton.spacedys.com/astdys/index.php?pc=1.1.3.0&n=Amycus

|access-date=2009-03-15

|archive-url=https://web.archive.org/web/20110526231319/http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.3.0&n=Amycus

|archive-date=2011-05-26

|url-status=dead}}

{{cite web

|date=2009-01-08

|title=Star occultation by asteroid 55576 Amycus

|publisher=IOTA (International Occultation Timing Association)

|author=Steve Preston

|url=http://www.asteroidoccultation.com/2009_02/0211_55576_17253_Summary.txt

|access-date=2009-12-28}}

{{Dead link|date=October 2010|bot=H3llBot}}

{{cite journal

|title=Bright Star Occultations by TNOs in 2014. J. Occultation Astronomy 2014-1.

|date=2013

|publisher=IOTA (International Occultation Timing Association)

|author=Hans-J. Bode

|author2=Filipe Braga Ribas

|author3=B. Sicardy}}

{{cite journal

|last=Horner |first= J.

|author2=Evans, N.W.

|author3=Bailey, M. E.

|title=Simulations of the Population of Centaurs I: The Bulk Statistics

|date=2004

|arxiv=astro-ph/0407400

|doi=10.1111/j.1365-2966.2004.08240.x

|volume=354

|journal=Monthly Notices of the Royal Astronomical Society

|issue= 3

|pages=798–810

|doi-access= free

|bibcode=2004MNRAS.354..798H|s2cid= 16002759

}}

}}