152 Atala
{{Short description|Main-belt asteroid}}
{{Use dmy dates|date=July 2020}}
{{Infobox planet
|minorplanet = yes
|name = 152 Atala
|image = 152Atala (Lightcurve Inversion).png
|image_scale =
|caption = A three-dimensional model of 152 Atala based on its light curve.
|symbol =
|background = #D6D6D6
|discovery_ref = [http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html Hardard's Numbered MPs]
|discoverer = P. P. Henry
|discovered = 2 November 1875
|discovery_site =
|mpc_name = (152) Atala
|mp_category = Main belt
|named_after = Atala
|alt_names = A875 VB
| pronounced={{IPAc-en|ə|'|t|ɑː|l|ə}}
{{IPA|fr|atala|lang}}
|orbit_ref = {{Cite web |url=http://ftp.lowell.edu/pub/elgb/astorb.html |website=astorb |title=The Asteroid Orbital Elements Database |publisher=Lowell Observatory }}
|epoch = 31 July 2016 (JD 2457600.5)
|aphelion = {{Convert|3.3855|AU|Gm|abbr=on|lk=on}}
|perihelion = {{Convert|2.8984|AU|Gm|abbr=on}}
|semimajor = {{Convert|3.1420|AU|Gm|abbr=on}}
|eccentricity = 0.077507
|inclination = 12.114°
|asc_node = 39.945°
|mean_anomaly = 52.593°
|arg_peri = 59.807°
|satellites =
|dimensions = 65 ± 8 km{{cite journal
|display-authors=6
|last=Ďurech
|first=Josef
|author2=Kaasalainen, Mikko
|author3=Herald, David
|author4=Dunham, David
|author5=Timerson, Brad
|author6=Hanuš, Josef
|author7=Frappa, Eric
|author8=Talbot, John
|author9=Hayamizu, Tsutomu
|author10=Warner, Brian D.
|author11=Pilcher, Frederick
|author12=Galád, Adrián
|title=Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes
|journal=Icarus
|volume=214
|issue=2
|pages=652–670
|date=2011
|url=http://astro.troja.mff.cuni.cz/projects/asteroids3D/download/durech_et_al_2011_occ_paper.pdf
|doi=10.1016/j.icarus.2011.03.016
|arxiv=1104.4227
|bibcode=2011Icar..214..652D
|access-date=26 January 2012
|archive-date=3 March 2016
|archive-url=https://web.archive.org/web/20160303214312/http://astro.troja.mff.cuni.cz/projects/asteroids3D/download/durech_et_al_2011_occ_paper.pdf
|url-status=dead
|mass = {{nowrap|(5.43 ± 1.24) × 1018 kg}}
|density =
|sidereal_day = 5.28-6.25 hours
|axial_tilt =
|pole_ecliptic_lat =
|pole_ecliptic_lon =
|albedo = 0.054
|temp_name1 =
|mean_temp_1 =
|max_temp_1 =
|temp_name2 =
|max_temp_2 =
|spectral_type = D[http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT SPIFF LCSUMPUB]
|abs_magnitude = 8.33
|mean_motion = {{Deg2DMS|0.17697|sup=ms}} / day
|observation_arc = 130.69 yr (47735 d)
|uncertainty = 0
|rotation = {{Convert|6.246|h|d|abbr=on|lk=on}}
|moid = {{Convert|1.93567|AU|Gm|abbr=on}}
|jupiter_moid = {{Convert|1.85235|AU|Gm|abbr=on}}
|tisserand = 3.171
}}
152 Atala is a large main belt asteroid that was discovered by brothers Paul Henry and Prosper Henry on 2 November 1875, but the discovery was credited to Paul. It is a type D asteroid, meaning that it is composed of carbon, organic rich silicates and possibly water ice.
The asteroid is named for the eponymous heroine of the 1801 novella Atala by François-René de Chateaubriand.{{Cite book |last=Schmadel |first=Lutz D.|authorlink=Lutz D. Schmadel|author2=International Astronomical Union |title=Dictionary of minor planet names |date=2003 |publisher=Springer-Verlag |location=Berlin; New York |isbn=978-3-540-00238-3 |page=29|url=https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA29}} The Henry brothers also named the last of their discoveries, 186 Celuta, after another Chateaubriand heroine.{{Cite book |last=Schmadel |first=Lutz D.|authorlink=Lutz D. Schmadel|author2=International Astronomical Union |title=Dictionary of minor planet names |date=2012 |edition=6th |publisher=Springer-Verlag |location=Berlin; New York |isbn=9783642297182 |page=29|url=https://books.google.com/books?id=aeAg1X7afOoC&q&pg=PA29|accessdate=4 April 2014}} Both Atala and Céluta are American Indian fictional characters.{{cite book |last=Chateaubriand |first=François-René |authorlink=François-René de Chateaubriand |title=Atala |date=1801}}; {{cite book |last=Chateaubriand |first=François-René |authorlink=François-René de Chateaubriand |title=René |date=1802}}
An occultation of a star by Atala was observed from Japan on 11 March 1994. Subsequent occultations have been observed as recently as 2006.{{citation needed|date=March 2019}}
Photometric of this asteroid made in 1981 gave a light curve with a period of 5.282 ± 0.004 hours with a brightness variation of 0.50 in magnitude.
References
{{Reflist|refs=
| first1 = Donald K.
| last1 = Yeomans
| title = 152 Atala
| work = JPL Small-Body Database Browser
| publisher = NASA Jet Propulsion Laboratory
| url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=152
| accessdate= 12 May 2016
| postscript= .}}
| first1 = B.
| last1 = Carry
| title = Density of asteroids
| work = Planetary and Space Science
| volume = 73
| pages = 98–118
|date=December 2012
| doi = 10.1016/j.pss.2012.03.009
| bibcode = 2012P&SS...73...98C
| postscript= .
|arxiv = 1203.4336 }} See Table 1.
| last1 = Schober
| first1 = H. J.
| title = The large C-type asteroids 146 Lucina and 410 Chloris, and the small S-type asteroids 152 Atala and 631 Philippina - Rotation periods and lightcurves
| journal = Astronomy and Astrophysics Supplement Series
| volume = 53
| pages = 71–75
|date=July 1983
| bibcode = 1983A&AS...53...71S
| postscript= .}}
}}
External links
- [http://iota.jhuapl.edu/mp152505.htm Occultation of TYC 5558-01048-1 by (152) Atala] on 2006 May 7 UT
- [https://archive.today/20130222093646/http://home.surewest.net/kheider/astro/152Atala_2007.gif (152) Atala near opposition 5 July 2007] (2.38AU from Earth)
- {{AstDys|151}}
- {{JPL small body}}
{{Minor planets navigator |151 Abundantia |number=152 |153 Hilda}}
{{Small Solar System bodies}}
{{Authority control}}
{{DEFAULTSORT:Atala}}
Category:Discoveries by Paul Henry and Prosper Henry
Category:François-René de Chateaubriand
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