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{{Short description|Main-belt asteroid}}
{{Use dmy dates|date=March 2020}}
{{Infobox planet
{{Infobox planet
|width = 25em
| minorplanet = yes
|background = #FFFFC0 | name=333 Badenia
| name = 333 Badenia
| background = #D6D6D6
| discoverer=[[Max Wolf]]
| image = 000333-asteroid shape model (333) Badenia.png
| discovered=August 22, 1892
| image_scale =
| alt_names=1892 A, A895 DC,<br>A911 CA, 1930 JD,<br>1932 TC, 1936 QQ,<br>1937 VB, 1950 BP1
| caption = Modelled shape of ''Badenia'' from its [[lightcurve]]
| named_after = [[Baden]]
| discovery_ref = &thinsp;<ref name="MPC-object" />
| mp_category=[[Asteroid belt|Main belt]] ([[Hygiea family]])
| discoverer = [[Max Wolf|M. F. Wolf]]
| epoch=30 January 2005 ([[Julian day|JD]] 2453400.5)
| discovery_site = [[Heidelberg-Königstuhl State Observatory|Heidelberg Obs.]]
| semimajor=467.419 Gm (3.125 [[Astronomical unit|AU]])
| discovered = 22 August 1892
| perihelion=389.041 Gm (2.601 AU)
| mpc_name = (333) Badenia
| aphelion=545.798 Gm (3.648 AU)
| alt_names = A892 QA{{·}}1930 JD<br />1932 TC{{·}}1936 QQ<br />1937 VB{{·}}{{mp|1950 BP|1}}<br />A895 DC{{·}}A911 CA<br />1892 A
| eccentricity=0.168
| pronounced = {{IPAc-en|b|ə|ˈ|d|iː|n|i|ə}}
| period=2017.262 d (5.52 [[Julian year (astronomy)|a]])
| named_after = {{nowrap|[[Grand Duchy of Baden]]}}<br />{{small|(Großherzogtum Baden)}}<ref name="springer" />
| inclination=3.794°
| mp_category = {{plainlist|
| asc_node=354.163°
* {{nowrap|[[main-belt]]&thinsp;<ref name="MPC-object" /><ref name="jpldata" />{{·}}{{small|([[Kirkwood gap|outer]])}}}}
| arg_peri=17.737°
* [[Background asteroid|background]]&thinsp;<ref name="AstDys-object" /><ref name="Ferret" />}}
| mean_anomaly=108.683°
| orbit_ref = &thinsp;<ref name="jpldata" />
| avg_speed=16.85 km/s
| epoch = 31 May 2020 ([[Julian day|JD]] 2459000.5)
| dimensions=78 km<sup>[http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab]</sup>
| uncertainty = 0
| mass=~3.5×10<sup>17</sup> kg ''(estimate)''
| observation_arc = 127.45 [[Julian year (astronomy)|yr]] (46,551 d)
| density=~1.4 g/cm³ ''(estimate)''<sup>[[#Krasinsky02|[3]]]</sup>
| aphelion = 3.6300 [[Astronomical unit|AU]]
| surface_grav=~0.015 m/s² ''(estimate)''
| perihelion = 2.6314 AU
| escape_velocity=~0.035 km/s ''(estimate)''
| semimajor = 3.1307 AU
| rotation=0.415 d <sup>[http://www.psi.edu/pds/archive/lc.html]</sup>
| eccentricity = 0.1595
| spectral_type=[[C-type asteroid]]
| period = 5.54 yr (2,023 d)
| abs_magnitude=9.46
| mean_anomaly = 20.070[[Degree (angle)|°]]
| albedo=0.0475 <sup>[[#IRAS|[1]]]</sup>
| mean_motion = {{Deg2DMS|0.1779|sup=ms}} / day
| single_temperature=~160 [[kelvin|K]]<br>''max:'' 248K (-26° C)}}
| inclination = 3.7393°
| asc_node = 353.16°
| arg_peri = 22.785°
| mean_diameter = {{plainlist|
* {{val|69.73|2.80|u=km}}<ref name="AKARI" />
* {{val|72.199|0.259|u=km}}<ref name="Mainzer-2016" />
* {{val|78.17|1.9|u=km}}<ref name="SIMPS" />}}
| density = {{val|1.4|ul=g/cm3|p=~}}<ref name="Krasinsky-2002" />
| rotation = {{val|9.862|0.001|ul=h}}<ref name="Pilcher-2017h" /><ref name="lcdb" />
| albedo = {{plainlist|
* {{val|0.0475}}<ref name="SIMPS" />
* {{val|0.057}}<ref name="Mainzer-2016" />
* {{val|0.061}}<ref name="AKARI" />}}
| spectral_type = {{plainlist|
* [[Tholen classification|Tholen]] {{=}} [[C-type asteroid|C]]:&thinsp;<ref name="jpldata" />
* [[Asteroid color indices|B–V]] {{=}} {{val|0.773|0.028}}<ref name="jpldata" />
* [[Asteroid color indices|U–B]] {{=}} {{val|0.401|0.042}}<ref name="jpldata" />}}
| abs_magnitude = 9.4<ref name="MPC-object" /><ref name="jpldata" />
}}


'''333 Badenia''' ({{IPAc-en|b|ə|ˈ|d|iː|n|i|ə}} {{respell|bə|DEE|nee-ə}}; ''[[Minor planet provisional designation|prov. designation]]:'' {{mp|A892 QA}} ''or'' {{mp|1892 A}}) is a large [[background asteroid]], approximately {{convert|72|km|mi|abbr=off|sigfig=2|sp=us}} in diameter, located the outer region of the [[asteroid belt]]. It was discovered on 22 August 1892, by astronomer [[Max Wolf]] at the [[Heidelberg-Königstuhl State Observatory]] in southwest Germany.<ref name="MPC-object" /> The carbonaceous [[C-type asteroid]] has a [[rotation period]] of 9.9 hours. It was named after the historical [[Grand Duchy of Baden]] that existed until 1918, and where the discovering observatory is located.<ref name="springer" /> ''Badenia'' was the first asteroid to receive a provisional designation.
'''333 Badenia''' ({{IPAc-en|icon|b|ə|ˈ|d|iː|n|i|ə}} {{respell|bə|DEE|nee-ə}}) is a large [[C-type asteroid|C-type]] (carbonaceous-type) [[asteroid]] in the outer [[asteroid belt]].


== Orbit and classification ==
It was discovered by [[Max Wolf]] on August 22, 1892 in [[Heidelberg]].


''Badenia'' is a non-[[Asteroid family|family]] asteroid of the main belt's [[Background asteroid|background population]] when applying the [[hierarchical clustering method]] to its [[proper orbital elements]].<ref name="AstDys-object" /><ref name="Ferret" /> It orbits the Sun in the [[Kirkwood gap|outer]] main-belt at a distance of 2.6–3.6&nbsp;[[Astronomical unit|AU]] once every 5 years and 6 months (2,023 days; [[semi-major axis]] of 3.13&nbsp;AU). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.16 and an [[orbital inclination|inclination]] of 4[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" />
==References==
#<div id="IRAS">[http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab Supplemental IRAS Minor Planet Survey]</div>
#[http://www.psi.edu/pds/archive/lc.html PDS lightcurve data]
#<div id="Krasinsky02">G. A. Krasinsky et al. ''Hidden Mass in the Asteroid Belt'', Icarus, Vol. 158, p.&nbsp;98 (2002).</div>


== Physical characteristics ==
{{Minor planets navigator|332 Siri|334 Chicago}}

In the [[Tholen classification]], ''Badenia'' is a common carbonaceous [[C-type asteroid]], though with a nosy spectrum (:).<ref name="jpldata" />

=== Rotation period ===

In April 2017, a rotational [[lightcurve]] of ''Badenia'' was obtained from [[Photometry (astronomy)|photometric]] observations by [[Frederick Pilcher]]. Lightcurve analysis gave a [[rotation period]] of {{val|9.862|0.001}} hours with a brightness variation of {{val|0.24|0.02}} [[Magnitude (astronomy)|magnitude]] ({{small|[[LCDB quality code|U=3]]}}).<ref name="Pilcher-2017h" /><ref name="lcdb" />

=== Diameter and albedo ===

According to the surveys carried out by the Infrared Astronomical Satellite [[IRAS]], the Japanese [[Akari (satellite)|Akari satellite]] and the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]], ''Badenia'' measures between 64.01 and 78.51 kilometers in diameter and its surface has an [[astronomical albedo|albedo]] between 0.047 and 0.061.<ref name="Ferret" /><ref name="AKARI" /><ref name="Mainzer-2016" /><ref name="SIMPS" /> The ''Collaborative Asteroid Lightcurve Link'' adopts the results from IRAS, that is, an albedo of 0.0475 and a diameter of 78.17 kilometers based on an [[absolute magnitude]] of 9.46.<ref name="lcdb" />

== References ==
{{reflist|30em|refs=

<ref name="jpldata">{{cite web
|type = 2020-02-04 last obs.
|title = JPL Small-Body Database Browser: 333 Badenia (A892 QA)
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000333
|publisher = [[Jet Propulsion Laboratory]]
|access-date = 11 March 2020}}</ref>

<ref name="springer">{{cite book
|title = Dictionary of Minor Planet Names
|url = https://archive.org/details/dictionaryminorp00schm
|url-access = limited
|last = Schmadel | first = Lutz D.
|publisher = Springer Berlin Heidelberg
|chapter = (333) Badenia
|page = [https://archive.org/details/dictionaryminorp00schm/page/n56 43]
|date = 2007
|doi = 10.1007/978-3-540-29925-7_334
|isbn = 978-3-540-00238-3}}</ref>

<ref name="MPC-object">{{cite web
|title = 333 Badenia (A892 QA)
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=333
|access-date = 11 March 2020}}</ref>

<ref name="lcdb">{{cite web
|title = LCDB Data for (333) Badenia
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=333
|access-date = 11 March 2020}}</ref>

<ref name="SIMPS">{{cite journal
|first1 = E. F. |last1 = Tedesco
|first2 = P. V. |last2 = Noah
|first3 = M. |last3 = Noah
|first4 = S. D. |last4 = Price
|date = October 2004
|title = IRAS Minor Planet Survey V6.0
|url = https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
|journal = NASA Planetary Data System
|volume = 12
|pages = IRAS-A-FPA-3-RDR-IMPS-V6.0
|bibcode = 2004PDSS...12.....T
|access-date = 11 March 2020}}</ref>

<ref name="AKARI">{{cite journal
|display-authors = 6
|first1 = Fumihiko |last1 = Usui
|first2 = Daisuke |last2 = Kuroda
|first3 = Thomas G. |last3 = Müller
|first4 = Sunao |last4 = Hasegawa
|first5 = Masateru |last5 = Ishiguro
|first6 = Takafumi |last6 = Ootsubo
|first7 = Daisuke |last7 = Ishihara
|first8 = Hirokazu |last8 = Kataza
|first9 = Satoshi |last9 = Takita
|first10 = Shinki |last10 = Oyabu
|first11 = Munetaka |last11 = Ueno
|first12 = Hideo |last12 = Matsuhara
|first13 = Takashi |last13 = Onaka
|date = October 2011
|title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
|journal = Publications of the Astronomical Society of Japan
|volume = 63
|issue = 5
|pages = 1117–1138
|bibcode = 2011PASJ...63.1117U
|doi = 10.1093/pasj/63.5.1117
|doi-access=
}} ([http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-source=J/PASJ/63/1117/acua_v1&Num=333 online], [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153])</ref>

<ref name="Mainzer-2016">{{cite journal
|display-authors = 6
|first1 = A. K. |last1 = Mainzer
|first2 = J. M. |last2 = Bauer
|first3 = R. M. |last3 = Cutri
|first4 = T. |last4 = Grav
|first5 = E. A. |last5 = Kramer
|first6 = J. R. |last6 = Masiero
|first7 = C. R. |last7 = Nugent
|first8 = S. M. |last8 = Sonnett
|first9 = R. A. |last9 = Stevenson
|first10 = E. L. |last10 = Wright
|date = June 2016
|title = NEOWISE Diameters and Albedos V1.0
|url = https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab
|journal = NASA Planetary Data System
|bibcode = 2016PDSS..247.....M
|access-date= 11 March 2020}}</ref>

<ref name="Pilcher-2017h">{{cite journal
|last1 = Pilcher |first1 = Frederick
|date = October 2017
|title = Rotation Period Determination for 46 Hestia, 118 Peitho, 333 Badenia, 356 Liguria, and 431 Nephele
|journal = Minor Planet Bulletin
|url = http://www.minorplanet.info/MPB/issues/MPB_44-4.pdf
|volume = 44
|issue = 4
|pages = 294–297
|bibcode = 2017MPBu...44..294P
|issn = 1052-8091}}</ref>
<!--
<ref name="geneva-obs">{{cite web
|title = Asteroids and comets rotation curves – (333) Badenia
|last = Behrend |first = Raoul
|publisher = Geneva Observatory
|url = http://obswww.unige.ch/~behrend/page1cou.html#000333
|access-date = 11 March 2020}}</ref>

<ref name="Blanco-2000a">{{cite journal
|last1 = Blanco |first1 = C.
|last2 = Di Martino |first2 = M.
|last3 = Riccioli |first3 = D.
|date = April 2000
|title = New rotational periods of 18 asteroids
|journal = Planetary and Space Science
|volume = 48
|issue = 4
|pages = 271–284
|bibcode = 2000P&SS...48..271B
|issn = 0032-0633
|doi = 10.1016/S0032-0633(99)00074-4}}</ref>

<ref name="Denchev-2000a">{{cite journal
|last1 = Denchev |first1 = P.
|last2 = Shkodrov |first2 = V.
|last3 = Ivanova |first3 = V.
|date = August 2000
|title = Synodic periods of asteroids 333, 402, 481, and 800
|journal = Planetary and Space Science
|volume = 48
|issue = 10
|pages = 983–986
|bibcode = 2000P&SS...48..983D
|issn = 0032-0633
|doi = 10.1016/S0032-0633(00)00066-0}}</ref>

<ref name="Aznar-2016c">{{cite journal
|display-authors = 6
|last1 = Aznar Macias |first1 = Amadeo
|last2 = Carreno Garcerain |first2 = Alfonso
|last3 = Arce Masego |first3 = Enrique
|last4 = Brines Rodriguez |first4 = Pedro
|last5 = Lozano de Haro |first5 = Juan
|last6 = Fornas Silva |first6 = Alvaro
|last7 = Fornas Silva |first7 = Gonzalo
|last8 = Mas Martinez |first8 = Vicente
|last9 = Rodrigo Chiner |first9 = Onofre
|last10 = Herrero Porta |first10 = David
|date = July 2016
|title = Twenty-one Asteroid Lightcurves at Group Observadores de Asteroides (OBAS): Late 2015 to Early 2016
|journal = Minor Planet Bulletin
|url = http://www.minorplanet.info/MPB/issues/MPB_43-3.pdf
|volume = 43
|issue = 3
|pages = 257–263
|bibcode = 2016MPBu...43..257A
|issn = 1052-8091}}</ref>

<ref name="Durech-2018d">{{cite journal
|last1 = Ďurech |first1 = J.
|last2 = Hanuš |first2 = J.
|date = November 2018
|title = Reconstruction of asteroid spin states from Gaia DR2 photometry
|journal = Astronomy and Astrophysics
|volume = 620
|page = A91
|bibcode = 2018A&A...620A..91D
|issn = 0004-6361
|doi = 10.1051/0004-6361/201834007
|arxiv = 1810.04485}}</ref>
-->
<ref name="Ferret">{{cite web
|title = Asteroid 333 Badenia
|work = Small Bodies Data Ferret
|url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=333+Badenia
|access-date = 11 March 2020}}</ref>

<ref name="AstDys-object">{{cite web
|title = Asteroid 333 Badenia – Proper Elements
|publisher = AstDyS-2, Asteroids – Dynamic Site
|url = https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=333
|access-date= 11 March 2020}}</ref>

<ref name="Krasinsky-2002">{{cite journal
|last1 = Krasinsky |first1 = G. A.
|last2 = Pitjeva |first2 = E. V.
|last3 = Vasilyev |first3 = M. V.
|last4 = Yagudina |first4 = E. I.
|date = July 2002
|title = Hidden Mass in the Asteroid Belt
|journal = Icarus
|volume = 158
|issue = 1
|pages = 98–105
|bibcode = 2002Icar..158...98K
|issn = 0019-1035
|doi = 10.1006/icar.2002.6837}}</ref>

}} <!-- end of reflist -->

== External links ==
* [http://www.minorplanet.info/PHP/OneAsteroidInfo.php Lightcurve Database Query] (LCDB), at ''www.minorplanet.info''
* [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
* [http://obswww.unige.ch/~behrend/page_cou.html Asteroids and comets rotation curves, CdR] – ''[[Geneva Observatory]]'', [[Raoul Behrend]]
* [http://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
* {{AstDys|333}}
* {{JPL small body}}

{{Minor planets navigator |332 Siri |number=333 |334 Chicago}}
{{Small Solar System bodies}}
{{Small Solar System bodies}}
{{Authority control}}


{{DEFAULTSORT:Badenia}}
{{DEFAULTSORT:Badenia}}
[[Category:Main Belt asteroids]]
[[Category:Background asteroids|000333]]
[[Category:Hygiea asteroids]]
[[Category:C-type asteroids]]
[[Category:Discoveries by Max Wolf]]
[[Category:Discoveries by Max Wolf]]
[[Category:Asteroids named for places]]
[[Category:Named minor planets]]
[[Category:Astronomical objects discovered in 1892]]
[[Category:C-type asteroids (Tholen)|000333]]
[[Category:Astronomical objects discovered in 1892|18920822]]

{{C-beltasteroid-stub}}

[[hy:(333) Բադենիա]]

Latest revision as of 20:36, 14 January 2024

333 Badenia
Modelled shape of Badenia from its lightcurve
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 August 1892
Designations
(333) Badenia
Pronunciation/bəˈdiːniə/
Named after
Grand Duchy of Baden
(Großherzogtum Baden)[2]
A892 QA · 1930 JD
1932 TC · 1936 QQ
1937 VB · 1950 BP1
A895 DC · A911 CA
1892 A
Orbital characteristics [3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc127.45 yr (46,551 d)
Aphelion3.6300 AU
Perihelion2.6314 AU
3.1307 AU
Eccentricity0.1595
5.54 yr (2,023 d)
20.070°
0° 10m 40.44s / day
Inclination3.7393°
353.16°
22.785°
Physical characteristics
  • 69.73±2.80 km[6]
  • 72.199±0.259 km[7]
  • 78.17±1.9 km[8]
Mean density
~1.4 g/cm3[9]
9.862±0.001 h[10][11]
9.4[1][3]

333 Badenia (/bəˈdiːniə/ bə-DEE-nee-ə; prov. designation: A892 QA or 1892 A) is a large background asteroid, approximately 72 kilometers (45 miles) in diameter, located the outer region of the asteroid belt. It was discovered on 22 August 1892, by astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory in southwest Germany.[1] The carbonaceous C-type asteroid has a rotation period of 9.9 hours. It was named after the historical Grand Duchy of Baden that existed until 1918, and where the discovering observatory is located.[2] Badenia was the first asteroid to receive a provisional designation.

Orbit and classification

[edit]

Badenia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the outer main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (2,023 days; semi-major axis of 3.13 AU). Its orbit has an eccentricity of 0.16 and an inclination of 4° with respect to the ecliptic.[3]

Physical characteristics

[edit]

In the Tholen classification, Badenia is a common carbonaceous C-type asteroid, though with a nosy spectrum (:).[3]

Rotation period

[edit]

In April 2017, a rotational lightcurve of Badenia was obtained from photometric observations by Frederick Pilcher. Lightcurve analysis gave a rotation period of 9.862±0.001 hours with a brightness variation of 0.24±0.02 magnitude (U=3).[10][11]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Badenia measures between 64.01 and 78.51 kilometers in diameter and its surface has an albedo between 0.047 and 0.061.[5][6][7][8] The Collaborative Asteroid Lightcurve Link adopts the results from IRAS, that is, an albedo of 0.0475 and a diameter of 78.17 kilometers based on an absolute magnitude of 9.46.[11]

References

[edit]
  1. ^ a b c d "333 Badenia (A892 QA)". Minor Planet Center. Retrieved 11 March 2020.
  2. ^ a b Schmadel, Lutz D. (2007). "(333) Badenia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 43. doi:10.1007/978-3-540-29925-7_334. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f g h "JPL Small-Body Database Browser: 333 Badenia (A892 QA)" (2020-02-04 last obs.). Jet Propulsion Laboratory. Retrieved 11 March 2020.
  4. ^ a b "Asteroid 333 Badenia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 11 March 2020.
  5. ^ a b c "Asteroid 333 Badenia". Small Bodies Data Ferret. Retrieved 11 March 2020.
  6. ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
  7. ^ a b c Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. Bibcode:2016PDSS..247.....M. Retrieved 11 March 2020.
  8. ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 11 March 2020.
  9. ^ Krasinsky, G. A.; Pitjeva, E. V.; Vasilyev, M. V.; Yagudina, E. I. (July 2002). "Hidden Mass in the Asteroid Belt". Icarus. 158 (1): 98–105. Bibcode:2002Icar..158...98K. doi:10.1006/icar.2002.6837. ISSN 0019-1035.
  10. ^ a b Pilcher, Frederick (October 2017). "Rotation Period Determination for 46 Hestia, 118 Peitho, 333 Badenia, 356 Liguria, and 431 Nephele" (PDF). Minor Planet Bulletin. 44 (4): 294–297. Bibcode:2017MPBu...44..294P. ISSN 1052-8091.
  11. ^ a b c "LCDB Data for (333) Badenia". Asteroid Lightcurve Database (LCDB). Retrieved 11 March 2020.
[edit]
Retrieved from "https://en.wikipedia.org/enwiki/w/index.php?title=333_Badenia&oldid=1195666526"