→In popular culture: rm not notable unsourced mention
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Added bibcode. | Use this bot. Report bugs. | Suggested by Abductive | Category:Periodic comets | #UCB_Category 13/174
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| discovery_date = January 17, 1948 |
| discovery_date = January 17, 1948 |
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| designations = 1961 IV; 1960m;<br/>1967 XIV; 1967k;<br/>1974 XI; 1974i;<br/>1986 VI; 1985q;<br/>1991 XVI; 1991s;<br/>46P/1948 A1;<br/>1947 XIII; 1948b;<br/>46P/1954 R2;<br/>1954 XI;<br/>1954j |
| designations = 1961 IV; 1960m;<br/>1967 XIV; 1967k;<br/>1974 XI; 1974i;<br/>1986 VI; 1985q;<br/>1991 XVI; 1991s;<br/>46P/1948 A1;<br/>1947 XIII; 1948b;<br/>46P/1954 R2;<br/>1954 XI;<br/>1954j |
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| orbit_ref = <ref name="MPC"/> |
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| epoch=September 3, 2002 (JDT 2452520.5)<!--- source: http://www.aerith.net/comet/catalog/0046P/2002.html ---> |
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| epoch = 2023-02-25<br/>(JDT 2460000.5) |
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| Earth_moid = {{Convert|0.068|AU|km|abbr=on}}<ref name=jpl-close/> |
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| semimajor = 3. |
| semimajor = 3.091 [[Astronomical Unit|AU]] |
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| perihelion = 1. |
| perihelion = 1.055AU |
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| aphelion = 5. |
| aphelion = 5.127AU |
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| eccentricity = 0. |
| eccentricity = 0.65867 |
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| period = 5. |
| period = 5.43 [[Julian year (astronomy)|yr]] |
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| inclination = 11. |
| inclination = 11.749° |
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| dimensions = {{val|1.4|u=km}}<ref name=arizona>{{Cite web|url=https://uanews.arizona.edu/story/ua-researcher-captures-rare-radar-images-comet-46pwirtanen|title = UA Researcher Captures Rare Radar Images of Comet 46P/Wirtanen|date = 20 December 2018}}</ref> |
| Earth_moid = {{Convert|0.071|AU|km|abbr=on}}<ref name=jpldata/> |
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| dimensions = {{val|1.4|u=km}} (radar)<ref name=arizona>{{Cite web|url=https://uanews.arizona.edu/story/ua-researcher-captures-rare-radar-images-comet-46pwirtanen|title = UA Researcher Captures Rare Radar Images of Comet 46P/Wirtanen|date = 20 December 2018}}</ref> |
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| rotation = 8.9 hours<ref name=arizona/> |
| rotation = 8.9 hours<ref name=arizona/> |
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| last_p = December 12, 2018<ref name=MPC/><br>July 9, 2013<ref name="NK2190">{{cite web|date=2010-04-09|title=46P/Wirtanen (NK 1909)|publisher=OAA Computing and Minor Planet Sections|author=Syuichi Nakano|author-link=Syuichi Nakano|url=http://www.oaa.gr.jp/~oaacs/nk/nk1909.htm|access-date=2012-02-18}}</ref><br />February 2, 2008 |
| last_p = December 12, 2018<ref name=MPC/><br />July 9, 2013<ref name="NK2190">{{cite web|date=2010-04-09|title=46P/Wirtanen (NK 1909)|publisher=OAA Computing and Minor Planet Sections|author=Syuichi Nakano|author-link=Syuichi Nakano|url=http://www.oaa.gr.jp/~oaacs/nk/nk1909.htm|access-date=2012-02-18}}</ref><br />February 2, 2008 |
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| next_p = 2024-May-19<ref name=MPC/> |
| next_p = 2024-May-19<ref name=MPC/> |
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}} |
}} |
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{| class=wikitable style="text-align:center; font-size:11px; float:right; margin:2px" |
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⚫ |
'''46P/Wirtanen''' is a small short-period [[comet]] with a current [[orbit]]al period of 5.4 years.<ref name="NASA-20191203" /><ref name="UM-20191203" /> It was the original target for close investigation by the ''[[Rosetta probe|Rosetta]]'' [[spacecraft]], planned by the [[European Space Agency]], but an inability to meet the [[launch window]] caused ''Rosetta'' to be sent to [[67P/Churyumov–Gerasimenko]] instead.<ref>{{cite journal |title=Rosetta Lander—Philae: Implications of an alternative mission |journal=Acta Astronautica |first1=S. |last1=Ulamec |first2=S. |last2=Espinasse |first3=B. |last3=Feuerbacher |first4=M. |last4=Hilchenbach |first5=D. |last5=Moura |first6=H. |last6=Rosenbauer |first7=H. |last7=Scheuerle |first8=R. |last8=Willnecker |display-authors=5 |volume=58 |issue=8 |pages=435–441 |date=April 2006 |doi=10.1016/j.actaastro.2005.12.009 |bibcode=2006AcAau..58..435U}}</ref> It belongs to the [[Jupiter]] family of comets, all of which have [[aphelion|aphelia]] between 5 and 6 [[astronomical unit|AU]]. Its diameter is estimated at {{convert|1. |
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|- bgcolor= style="font-size: smaller;" |
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| colspan="8" style="text-align:center;"|'''Perihelion distance<br/>at different epochs'''<ref name="Kinoshita"/> |
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|- |
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! [[Epoch (astronomy)|Epoch]] !! [[Perihelion]]<br/>([[Astronomical unit|AU]]) |
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|- |
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| 1967 || 1.61 |
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|- |
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| 1974 || 1.26 |
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|- |
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| 1986 || 1.08 |
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|- |
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| 2013 || 1.05 |
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|- |
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| 2035 || 1.08 |
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|- |
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| 2046 || 1.22 |
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|- |
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| 2059 || 1.98 |
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|- |
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| 2095 || 2.01 |
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|} |
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⚫ | '''46P/Wirtanen''' is a small short-period [[comet]] with a current [[orbit]]al period of 5.4 years.<ref name="NASA-20191203" /><ref name="UM-20191203" /> It was the original target for close investigation by the ''[[Rosetta probe|Rosetta]]'' [[spacecraft]], planned by the [[European Space Agency]], but an inability to meet the [[launch window]] caused ''Rosetta'' to be sent to [[67P/Churyumov–Gerasimenko]] instead.<ref>{{cite journal |title=Rosetta Lander—Philae: Implications of an alternative mission |journal=Acta Astronautica |first1=S. |last1=Ulamec |first2=S. |last2=Espinasse |first3=B. |last3=Feuerbacher |first4=M. |last4=Hilchenbach |first5=D. |last5=Moura |first6=H. |last6=Rosenbauer |first7=H. |last7=Scheuerle |first8=R. |last8=Willnecker |display-authors=5 |volume=58 |issue=8 |pages=435–441 |date=April 2006 |doi=10.1016/j.actaastro.2005.12.009 |bibcode=2006AcAau..58..435U}}</ref> It belongs to the [[Jupiter]] family of comets, all of which have [[aphelion|aphelia]] between 5 and 6 [[astronomical unit|AU]]. Its diameter is estimated at {{convert|1.4|km|mi|sigfig=1}}. In December 2019, astronomers reported capturing an outburst of the comet in substantial detail by the [[TESS|TESS space telescope]].<ref name="NASA-20191203">{{cite news |author=Goddard Space Flight Center |author-link=Goddard Space Flight Center |title=NASA's exoplanet-hunting mission catches a natural comet outburst in unprecedented detail |url=https://www.eurekalert.org/pub_releases/2019-12/nsfc-nem120319.php |date=3 December 2019 |work=[[EurekAlert!]] |access-date=3 December 2019 }}</ref><ref name="UM-20191203">{{cite news |author=University of Maryland |author-link=University of Maryland |title=UMD astronomers catch a natural comet outburst in unprecedented detail - Data from NASA's Transiting Exoplanet Survey Satellite (TESS) reveal start-to-finish sequence of an outburst from comet 46P/Wirtanen |url=https://www.eurekalert.org/pub_releases/2019-12/uom-uac120319.php |date=3 December 2019 |work=[[EurekAlert!]] |access-date=3 December 2019 }}</ref> |
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== Discovery == |
== Discovery == |
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== Perihelion passages == |
== Perihelion passages == |
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The July 2013 perihelion passage was not favorable, only reaching a magnitude of 14.7.<ref name="Comet 46P/Wirtanen Information">{{Cite web|url=https://theskylive.com/46p-info|title=Comet 46P/Wirtanen Information|website=theskylive.com|access-date=2017-11-26}}</ref> Between January 23 and September 26 of 2013, the comet had an [[Elongation (astronomy)|elongation]] less than 20 degrees from the Sun. |
The July 2013 perihelion passage was not favorable, only reaching a magnitude of 14.7.<ref name="Comet 46P/Wirtanen Information">{{Cite web|url=https://theskylive.com/46p-info|title=Comet 46P/Wirtanen Information|website=theskylive.com|access-date=2017-11-26}}</ref> Between January 23 and September 26 of 2013, the comet had an [[Elongation (astronomy)|elongation]] less than 20 degrees from the Sun. |
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On 16 December 2018 the comet passed {{Convert|0.07746|AU|e6km e6mi LD|abbr=unit|lk=on|sigfig=3}} from Earth,<ref name=jpldata/> marking one of the 10 closest comet flybys of Earth in 70 years.<ref name=JPL-7306/> The comet reached an estimated magnitude of 3.9,<ref>{{cite web |title=Brightest comets seen since 1935 |url=http://www.icq.eps.harvard.edu/brightest.html |website=www.icq.eps.harvard.edu |access-date=20 April 2023}}</ref> making this pass the brightest one predicted, and the brightest close approach for the next 20 years.<ref name="Comet 46P/Wirtanen Information"/> The comet experienced six outbursts, with the comet brightening by −0.2 to −1.6 magnitudes.<ref>{{cite journal |last1=Kelley |first1=Michael S. P. |last2=Farnham |first2=Tony L. |last3=Li |first3=Jian-Yang |last4=Bodewits |first4=Dennis |last5=Snodgrass |first5=Colin |last6=Allen |first6=Johannes |last7=Bellm |first7=Eric C. |last8=Coughlin |first8=Michael W. |last9=Drake |first9=Andrew J. |last10=Duev |first10=Dmitry A. |last11=Graham |first11=Matthew J. |last12=Kupfer |first12=Thomas |last13=Masci |first13=Frank J. |last14=Reiley |first14=Dan |last15=Walters |first15=Richard |last16=Dominik |first16=M. |last17=Jørgensen |first17=U. G. |last18=Andrews |first18=A. E. |last19=Bach-Møller |first19=N. |last20=Bozza |first20=V. |last21=Burgdorf |first21=M. J. |last22=Campbell-White |first22=J. |last23=Dib |first23=S. |last24=Fujii |first24=Y. I. |last25=Hinse |first25=T. C. |last26=Hundertmark |first26=M. |last27=Khalouei |first27=E. |last28=Longa-Peña |first28=P. |last29=Rabus |first29=M. |last30=Rahvar |first30=S. |last31=Sajadian |first31=S. |last32=Skottfelt |first32=J. |last33=Southworth |first33=J. |last34=Tregloan-Reed |first34=J. |last35=Unda-Sanzana |first35=E. |display-authors=5|title=Six Outbursts of Comet 46P/Wirtanen |journal=The Planetary Science Journal |date=1 August 2021 |volume=2 |issue=4 |pages=131 |doi=10.3847/PSJ/abfe11|arxiv=2105.05826 |doi-access=free |bibcode=2021PSJ.....2..131K }}</ref> |
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On 16 December 2018 the comet passed {{convert|0.0774|AU|km mi|abbr=on|lk=on}} (≈30.1 [[Lunar distance (astronomy)|LD]]) from Earth,<ref name=jpl-close/> reaching an estimated magnitude of 4.2,<ref>{{Cite web|url=https://www.timeanddate.com/astronomy/comets/46p-wirtanen-2018.html|title=Look Up! Comet 46P/Wirtanen to Flyby in December 2018|website=timeanddate.com|access-date=2018-12-06}}</ref> making this pass the brightest one predicted, and the brightest close approach for the next 20 years.<ref name="Comet 46P/Wirtanen Information"/> Its magnitude could peak as bright as magnitude 3 near its December 16, 2018 closest approach.<ref>{{Cite web|url=http://www.physics-astronomy.org/2018/10/brightest-comet-of-2018-to-light-up-sky.html|title = Brightest Comet of 2018 to Light up the Sky in December}}</ref> It was one of the 10 closest comet flybys of Earth in 70 years.<ref name=JPL-7306/> |
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The 2018 close approach, combined with Wirtanen's brightness provides an opportunity to study a potential future spacecraft mission target in detail. A worldwide observing campaign<ref>{{Cite web|url=http://wirtanen.astro.umd.edu/|title=The Comet Wirtanen Observing Campaign|website=wirtanen.astro.umd.edu|access-date=2018-06-05}}</ref> |
The 2018 close approach, combined with Wirtanen's brightness provides an opportunity to study a potential future spacecraft mission target in detail. A worldwide observing campaign<ref>{{Cite web|url=http://wirtanen.astro.umd.edu/|title=The Comet Wirtanen Observing Campaign|website=wirtanen.astro.umd.edu|access-date=2018-06-05}}</ref> was organized to capitalize on the favorable circumstances of the 2018 apparition. |
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<gallery mode="packed"> |
<gallery mode="packed"> |
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File:C46P-sky.png|Path of 46P across the sky during 2018. Its size shown is inversely proportional to its distance. |
File:C46P-sky.png|Path of 46P across the sky during 2018. Its size shown is inversely proportional to its distance. |
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}}</ref> |
}}</ref> |
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== Associated |
== Associated meteor showers == |
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⚫ | Russian forecaster Mikhail Maslov had predicted that the [[Earth's orbit]] would cross Comet Wirtanen's debris stream as many as four times between December 10 and December 14, 2012. As there had not previously been an encounter with this debris stream, it was not certain whether or not a [[meteor shower]] would be visible from Earth, but there was speculation that a shower with as many as 30 meteors per hour might occur.<ref>{{cite web|title=A New Meteor Shower in December?|url=https://science.nasa.gov/science-news/science-at-nasa/2012/11dec_newshower/|publisher=NASA|access-date=2012-12-13}}</ref> |
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=== 2023 === |
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Close approaches to Jupiter in 1972 and 1984 moved the comet's orbit closer to Earth, and as of [[Epoch (astronomy)|epoch]] 2018 the comet has an Earth–[[Minimum orbit intersection distance|MOID]] of {{Convert|0.071|AU|e6km e6mi LD|abbr=unit|lk=on}}.<ref name=jpldata/> In 2023 Earth is expected to pass through a denser part of the 1974 [[Meteor shower#Origin of meteoroid streams|meteoroid stream]] than Earth did in 2007.<ref name=IMCCE2023/> The meteors would make [[atmospheric entry]] (Ve) at a relatively slow 15 km/s (10.3 km/s (Vg) before the influence of Earth's gravity). The [[Radiant (meteor shower)|radiant]] is near the southern constellation of [[Sculptor (constellation)|Sculptor]]. |
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{| class="wikitable" style="text-align: center; font-size: 0.9em;" |
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|+Possible meteoroid stream activity<ref name=IMCCE2023/> |
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! Date |
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! [[Meteor shower#Origin of meteoroid streams|Stream]] |
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|- |
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| 2007 || 1974 |
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|- |
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| 2018 || 1980 |
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|- |
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| 2023-December-12 10:54 UT || 1974 |
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|} |
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=== 2012 === |
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⚫ | Russian forecaster Mikhail Maslov had predicted that the [[Earth's orbit]] would cross Comet Wirtanen's debris stream as many as four times between December 10 and December 14, 2012. As there had not previously been an encounter with this debris stream, it was not certain whether or not a [[meteor shower]] would be visible from Earth, but there was speculation that a shower with as many as 30 meteors per hour might occur.<ref>{{cite web|title=A New Meteor Shower in December?|url=https://science.nasa.gov/science-news/science-at-nasa/2012/11dec_newshower/|publisher=NASA|access-date=2012-12-13 |archive-url=https://web.archive.org/web/20121212184725/https://science.nasa.gov/science-news/science-at-nasa/2012/11dec_newshower/ |archive-date=2012-12-12 |url-status=dead }}</ref> |
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Observers in Australia reported that on the night of December 14, 2012, as many as a dozen meteors were seen emanating from the predicted radiant in the constellation of [[Pisces (constellation)|Pisces]].<ref>{{cite web|title=Comet Wirtanen meteors report|url=http://www.iceinspace.com.au/forum/showthread.php?p=925959|publisher=IceInSpace|access-date=2012-12-17}}</ref> |
Observers in Australia reported that on the night of December 14, 2012, as many as a dozen meteors were seen emanating from the predicted radiant in the constellation of [[Pisces (constellation)|Pisces]].<ref>{{cite web|title=Comet Wirtanen meteors report|url=http://www.iceinspace.com.au/forum/showthread.php?p=925959|publisher=IceInSpace|access-date=2012-12-17}}</ref> |
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|url=https://www.minorplanetcenter.net/db_search/show_object?object_id=46P |
|url=https://www.minorplanetcenter.net/db_search/show_object?object_id=46P |
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|publisher=[[Minor Planet Center]] |
|publisher=[[Minor Planet Center]] |
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|access-date= |
|access-date=2023-10-01}}</ref> |
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<ref name= |
<ref name="Kinoshita">{{cite web |
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|title=46P/Wirtanen past, present and future orbital elements |
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⚫ |
|type=last observation: |
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|url=http://jcometobs.web.fc2.com/pcmtn/0046p.htm |
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⚫ | |||
|work=Comet Orbit |
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⚫ |
|url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=46P;orb=1;cad=1 |
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|first=Kazuo |last=Kinoshita |
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⚫ | |||
|date=2019-06-09 |
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|archive-url=https://web.archive.org/web/20120422080321/http://jcometobs.web.fc2.com/pcmtn/0046p.htm |
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|archive-date=2012-04-22 |
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|url-status=live |
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⚫ | |||
<ref name=jpldata>{{cite web |
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⚫ | |type=last observation: 2019-07-01; [[Observation arc|arc]]: 1.15 years |
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⚫ | |||
|url=https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=46P&view=OPC |
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⚫ | |archive-url=https://web.archive.org/web/20210723152712/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=46P;orb=1;cad=1 |
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|archive-date=2021-07-23 |
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|url-status=live |
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|access-date=2023-10-01}}</ref> |
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<ref name=JPL-7306>{{cite web |
<ref name=JPL-7306>{{cite web |
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Line 92: | Line 146: | ||
|publisher=JPL |
|publisher=JPL |
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|access-date=2019-03-03}}</ref> |
|access-date=2019-03-03}}</ref> |
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<ref name=IMCCE2023>{{cite web |
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|title=A new meteor shower caused by comet 46P/Wirtanen |
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|url=https://www.imcce.fr/recherche/campagnes-observations/meteors/2023wir |
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|publisher=IMCCE |
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|access-date=2023-10-01}}</ref> |
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}} <!-- end of reflist--> |
}} <!-- end of reflist--> |
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{{2018 in space}} |
{{2018 in space}} |
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{{PeriodicComets Navigator|45P/Honda–Mrkos–Pajdušáková|47P/Ashbrook–Jackson}} |
{{PeriodicComets Navigator|45P/Honda–Mrkos–Pajdušáková|47P/Ashbrook–Jackson}} |
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{{Authority control}} |
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{{DEFAULTSORT:Wirtanen}} |
{{DEFAULTSORT:Wirtanen}} |
Discovery | |
---|---|
Discovered by | Carl A. Wirtanen |
Discovery date | January 17, 1948 |
Designations | |
1961 IV; 1960m; 1967 XIV; 1967k; 1974 XI; 1974i; 1986 VI; 1985q; 1991 XVI; 1991s; 46P/1948 A1; 1947 XIII; 1948b; 46P/1954 R2; 1954 XI; 1954j | |
Orbital characteristics[1] | |
Epoch | 2023-02-25 (JDT 2460000.5) |
Aphelion | 5.127 AU |
Perihelion | 1.055 AU |
Semi-major axis | 3.091 AU |
Eccentricity | 0.65867 |
Orbital period | 5.43 yr |
Inclination | 11.749° |
Last perihelion | December 12, 2018[1] July 9, 2013[2] February 2, 2008 |
Next perihelion | 2024-May-19[1] |
Earth MOID | 0.071 AU (10,600,000 km)[3] |
Physical characteristics | |
Dimensions | 1.4 km (radar)[4] |
8.9 hours[4] |
Perihelion distance at different epochs[5] | |||||||
Epoch | Perihelion (AU) | ||||||
---|---|---|---|---|---|---|---|
1967 | 1.61 | ||||||
1974 | 1.26 | ||||||
1986 | 1.08 | ||||||
2013 | 1.05 | ||||||
2035 | 1.08 | ||||||
2046 | 1.22 | ||||||
2059 | 1.98 | ||||||
2095 | 2.01 |
46P/Wirtanen is a small short-period comet with a current orbital period of 5.4 years.[6][7] It was the original target for close investigation by the Rosetta spacecraft, planned by the European Space Agency, but an inability to meet the launch window caused Rosetta to be sent to 67P/Churyumov–Gerasimenko instead.[8] It belongs to the Jupiter family of comets, all of which have aphelia between 5 and 6 AU. Its diameter is estimated at 1.4 kilometres (0.9 mi). In December 2019, astronomers reported capturing an outburst of the comet in substantial detail by the TESS space telescope.[6][7]
46P/Wirtanen was discovered photographically on January 17, 1948, by the American astronomer Carl A. Wirtanen.[9] The plate was exposed on January 15 during a stellar proper motion survey for the Lick Observatory. Due to a limited number of initial observations, it took more than a year to recognize this object as a short-period comet.
The July 2013 perihelion passage was not favorable, only reaching a magnitude of 14.7.[10] Between January 23 and September 26 of 2013, the comet had an elongation less than 20 degrees from the Sun.
On 16 December 2018 the comet passed 0.07746 AU (11.6 million km; 7.20 million mi; 30.1 LD) from Earth,[3] marking one of the 10 closest comet flybys of Earth in 70 years.[11] The comet reached an estimated magnitude of 3.9,[12] making this pass the brightest one predicted, and the brightest close approach for the next 20 years.[10] The comet experienced six outbursts, with the comet brightening by −0.2 to −1.6 magnitudes.[13]
The 2018 close approach, combined with Wirtanen's brightness provides an opportunity to study a potential future spacecraft mission target in detail. A worldwide observing campaign[14] was organized to capitalize on the favorable circumstances of the 2018 apparition.
The comet was the target for the proposed Comet Hopper mission, which reached the finalist stage in the NASA Discovery program. It was one of only three missions in that selection to have a more detailed study. The selection process was ultimately won in 2012 by the InSight mission, a Mars lander. The Comet Hopper was designed to use the ASRG, the Advanced Stirling Radioisotope Generator.
The Comet Hopper mission, if it were selected, would have had multiple science goals over the 7.3 years of its nominal lifetime. At roughly 4.5 AU the spacecraft would rendezvous with Comet Wirtanen and begin to map the spatial heterogeneity of surface solids as well as gas and dust emissions from the coma - the nebulous envelope around the nucleus of a comet. The remote mapping would also allow for any nucleus structure, geologic processes, and coma mechanisms to be determined. After arriving at the comet, the spacecraft would approach and land, then subsequently hop to other locations on the comet. As the comet approached the Sun, the spacecraft would land and hop multiple times.[16] The final landing would occur at 1.5 AU. As the comet approached the Sun and became more active, the spacecraft would be able to record surface changes.[17]
Also, 46P/Wirtanen was the original destination of the European Space Agency's Rosetta spacecraft mission, but launch delays meant that the comet was no longer easily reachable and another periodic comet, 67P/Churyumov–Gerasimenko, was chosen as the mission's target instead.[18][19]
Close approaches to Jupiter in 1972 and 1984 moved the comet's orbit closer to Earth, and as of epoch 2018 the comet has an Earth–MOID of 0.071 AU (10.6 million km; 6.6 million mi; 28 LD).[3] In 2023 Earth is expected to pass through a denser part of the 1974 meteoroid stream than Earth did in 2007.[20] The meteors would make atmospheric entry (Ve) at a relatively slow 15 km/s (10.3 km/s (Vg) before the influence of Earth's gravity). The radiant is near the southern constellation of Sculptor.
Date | Stream |
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2007 | 1974 |
2018 | 1980 |
2023-December-12 10:54 UT | 1974 |
Russian forecaster Mikhail Maslov had predicted that the Earth's orbit would cross Comet Wirtanen's debris stream as many as four times between December 10 and December 14, 2012. As there had not previously been an encounter with this debris stream, it was not certain whether or not a meteor shower would be visible from Earth, but there was speculation that a shower with as many as 30 meteors per hour might occur.[21]
Observers in Australia reported that on the night of December 14, 2012, as many as a dozen meteors were seen emanating from the predicted radiant in the constellation of Pisces.[22]
2018 in space
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2019 » | ||
Space probe launches |
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Impact events |
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Selected NEOs |
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Exoplanets |
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Discoveries |
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Novae |
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Comets |
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Space exploration |
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Numbered comets | ||
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46P/Wirtanen | Next 47P/Ashbrook–Jackson |