Asteroïde: Verskil tussen weergawes

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[[Lêer:(253) mathilde.jpg|duimnael|270px|links|253 Mathilde is 'n asteroïde met ’n deursnee van sowat 50 km.]]
[[Beeld:Asteroid Belt.svg|thumb|’n Diagram van die Sonnestelsel se asteroïdegordel.]]
Daar is miljoene asteroïdes, waarvan baie vermoedelik die oorblyfsels is van [[planetesimale]], liggame in die jong Son se [[sonnewel]] wat nooit groot genoeg geword het om [[planete]] te vorm nie.<ref>{{cite web |website=CNEOS |title=Frequently Asked Questions (FAQs) – What Are Asteroids And Comets? |url=http://neo.jpl.nasa.gov/faq/#ast |accessdate=13 September 2010 |archiveurl= https://web.archive.org/web/20100909210213/http://neo.jpl.nasa.gov/faq/ |archivedate= 9 September 2010 <!--DASHBot-->| deadurl= nourl-status-live}}</ref> Die oorgrote meerderheid van bekende asteroïdes kom voor in die hoofasteroïdegordel tussen die wentelbane van [[Mars]] en Jupiter, of deel ’n wentelbaan met Jupiter (die [[Trojaan (sterrekunde)|Jupiter-trojane]]). Daar is egter taamlik groot families asteroïdes met ander wentelbane, insluitende die [[naby-aarde-voorwerp]]e. Individuele asteroïdes word geklassifiseer volgens hul kenmerkende [[Emissielyn|spektra]]. Die meeste val in drie hoofgroepe: C-, M- en S-tipe asteroïdes. Hulle is genoem na en word gewoonlik verbind met onderskeidelik [[koolstof]], [[metaal]] en [[silikaat]] (klipagtig). Asteroïdes se groottes wissel aansienlik; die grootste een, [[Ceres (dwergplaneet)|Ceres]], se deursnee is amper 1&nbsp;000&nbsp;km.
 
Asteroïdes verskil van komete en [[meteoroïde]]s. Die verskil tussen asteroïdes en komete is hul samestelling: Komete bestaan hoofsaaklik uit stof en ys en asteroïdes uit rots en minerale. Laasgenoemde het nader aan die Son ontstaan en bevat dus nie ys nie.<ref>{{cite web |title=What is the difference between an asteroid and a comet?|url=http://coolcosmos.ipac.caltech.edu/ask/181-What-is-the-difference-between-an-asteroid-and-a-comet- |website=Cool Cosmos |publisher=Infrared Processing and Analysis Center |accessdate=13 Augustus 2016}}</ref> Die verskil tussen asteroïdes en meteoroïdes is hul grootte: Meteoroïdes het ’n deursnee van ’n meter of kleiner, terwyl asteroïdes se deursnee groter as ’n meter is.<ref name=Rubin2010>{{cite journal |last1=Rubin |first1=Alan E. |last2=Grossman |first2=Jeffrey N. |title=Meteorite and meteoroid: new comprehensive definitions |journal=Meteoritics and Planetary Science |date=Januarie 2010 |volume=45 |issue=1 |pages=114–122 |bibcode=2010M&PS...45..114R |doi=10.1111/j.1945-5100.2009.01009.x |doi-access=free}}</ref> Meteoroïdes kan dieselfde samestelling as óf asteroïdes óf komete hê.<ref name="Universe Today">{{cite web |title=What is the difference between asteroids and meteorites? |url=http://www.universetoday.com/36398/what-is-the-difference-between-asteroids-and-meteorites/ |website=Universe Today |last=Atkinson |first=Nancy |date=2 Junie 2015 |accessdate=13 Augustus 2016}}</ref>
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Die [[Verenigde Nasies]] het [[30 Junie]] as Internasionale Asteroïdedag verklaar om die publiek oor asteroïdes op te voed. Dié datum herdenk die [[Toengoeska-voorval|Toengoeska-asteroïde-impak]] op 30 Junie 1908 in [[Siberië]], [[Rusland]].<ref>{{cite press release |url=http://www.unoosa.org/oosa/en/informationfor/media/2016-unis-os-478.html |title=United Nations General Assembly proclaims 30 June as International Asteroid Day |date=7 Desember 2016 |id=UNIS/OS/478 |website=United Nations Office for Outer Space Affairs}}</ref><ref>{{cite web |url=https://www.un.org/ga/search/view_doc.asp?symbol=A/71/492 |others=Rapporteur: Awale Ali Kullane |title=International cooperation in the peaceful uses of outer space |date=25 October 2016 |access-date=6 Desember 2016 |website=United Nations}}</ref>
 
In April 2018 het die B612 Foundation, wat hom onder meer toespits op verdediging teen asteroïdes, berig "die kans is 100&nbsp;persent dat ons deur ’n verwoestende asteroïde getref sal word, maar ons is nie 100&nbsp;persent seker wanneer nie".<ref name="DS-20180428">{{cite news |last=Harper |first=Paul |title=Earth will be hit by asteroid with 100% Certainty ...experts have warned it is "100pc certain" Earth will be devastated by an asteroid as millions are hurling towards the planet undetected |url=https://www.dailystar.co.uk/news/world-news/699177/Asteroids-earth-space-apocalypse-meteor-B612-Foundation |date=28 April 2018 |work=Daily Star |accessdate=26 November 2018 }}</ref><ref name="INQ-20180428">{{cite news |last=Homer |first=Aaron |title=Earth Will Be Hit By An Asteroid With 100 Percent Certainty, Says Space-Watching Group B612 – The group of scientists and former astronauts is devoted to defending the planet from a space apocalypse. |url=https://www.inquisitr.com/4881237/earth-will-be-hit-by-an-asteroid-with-100-percent-certainty-says-space-watching-group-b612/ |date=28 April 2018 |work=Inquisitr |accessdate=26 November 2018 }}</ref> Ook die fisikus [[Stephen Hawking]] het in 2018 in sy laaste boek, ''Brief Answers to the Big Questions'', gemeen ’n asteroïdebotsing is die grootste bedreiging wat ons planeet in die gesig staar.<ref name="WP-20181015">{{cite news |last=Stanley-Becker |first=Isaac |title=Stephen Hawking feared race of ‘superhumans’ able to manipulate their own DNA |url=https://www.washingtonpost.com/news/morning-mix/wp/2018/10/15/stephen-hawking-feared-race-of-superhumans-able-to-manipulate-their-own-dna/ |date=15 Oktober 2018 |work=The Washington Post |accessdate=26 November 2018 }}</ref><ref name="QZ-20181014">{{cite web |last=Haldevang |first=Max de |title=Stephen Hawking left us bold predictions on AI, superhumans, and aliens |url=https://qz.com/1423685/stephen-hawking-says-superhumans-will-take-over-ai-is-a-threat-and-humans-will-conquer-space/ |date=14 Oktober 2018 |work=Quartz |accessdate=26 November 2018 }}</ref><ref name="NYT-20180618">{{cite news |last=Bogdan |first=Dennis |title=\Better Way To Avoid Devastating Asteroids Needed? |url=https://www.nytimes.com/2018/06/14/science/asteroids-nasa-nathan-myhrvold.html#permid=27500228:27506217 |date=18 Junie 2018 |work=The New York Times |deadurl=nourl-status-live |archiveurl= |archivedate= |accessdate=26 November 2018 }}</ref>
 
In Junie 2018 het die [[VSA]] se nasionale wetenskap-en-tegnologieraad gewaarsku dat Amerika onvoorbereid op ’n asteroïde-impak is. Die raad het die "[https://www.whitehouse.gov/wp-content/uploads/2018/06/National-Near-Earth-Object-Preparedness-Strategy-and-Action-Plan-23-pages-1MB.pdf National Near-Earth Object Preparedness Strategy Action Plan]" ontwikkel en uitgereik om beter daarop voor te berei.<ref name="WH-20180621">{{cite web |author=Staff |title=National Near-Earth Object Preparedness Strategy Action Plan |url=https://www.whitehouse.gov/wp-content/uploads/2018/06/National-Near-Earth-Object-Preparedness-Strategy-and-Action-Plan-23-pages-1MB.pdf |format=PDF |date=21 June 2018 |work=White House |accessdate=22 June 2018 }}</ref><ref name="GIZ-20180621">{{cite news |last=Mandelbaum |first=Ryan F. |title=America Isn't Ready to Handle a Catastrophic Asteroid Impact, New Report Warns |url=https://gizmodo.com/america-isnt-ready-to-handle-a-catastrophic-asteroid-im-1827014709 |date=21 June 2018 |work=Gizmodo |accessdate=22 Junie 2018 }}</ref><ref name="ICARUS-220180522">{{cite journal |last=Myhrvold |first=Nathan |authorlink=Nathan Myhrvold |title=An empirical examination of WISE/NEOWISE asteroid analysis and results |url=https://www.sciencedirect.com/science/article/pii/S0019103516307643 |date=22 Mei 2018 |journal=Icarus|volume=314 |pages=64–97 |doi=10.1016/j.icarus.2018.05.004 |accessdate=22 June 2018 |bibcode=2018Icar..314...64M }}</ref><ref name="NYT-20180614c">{{cite news |last=Chang |first=Kenneth |title=Asteroids and Adversaries: Challenging What NASA Knows About Space Rocks |url=https://www.nytimes.com/2018/06/14/science/asteroids-nasa-nathan-myhrvold.html#permid=27500228:27506217 |date=14 Junie 2018 |work=The New York Times |accessdate=22 Junie 2018 }}</ref><ref name="NYT-20180614">{{cite news |last=Chang |first=Kenneth |title=Asteroids and Adversaries: Challenging What NASA Knows About Space Rocks |quote= Two years ago, NASA dismissed and mocked an amateur’s criticisms of its asteroids database. Now Nathan Myhrvold is back, and his papers have passed peer review. |url=https://www.nytimes.com/2018/06/14/science/asteroids-nasa-nathan-myhrvold.html |date=14 Junie 2018 |work=The New York Times |accessdate=26 November 2018 }}</ref> Volgens kennersgetuienis in 2013 in die Amerikaanse kongres het [[Nasa]] minstens vyf jaar van voorbereiding nodig voordat ’n sending van stapel gestuur kan word om ’n asteroïde te onderskep.<ref name="US-Congress-20130410">{{cite web |author=U.S.Congress |title=Threats From Space: a Review of U.S. Government Efforts to Track and mitigate Asteroids and Meteors (Part I and Part II) – Hearing Before the Committee on Science, Space, and Technology House of Representatives One Hundred Thirteenth Congress First Session |url=http://www.gpo.gov/fdsys/pkg/CHRG-113hhrg80552/pdf/CHRG-113hhrg80552.pdf |date=19 Maart 2013 |page=147 |work=United States Congress |accessdate=26 November 2018 }}</ref>
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| url=http://neo.jpl.nasa.gov/programs/
| title=Near Earth Object Search Programs
| publisher=NASA | accessdate=15 April 2008 | archiveurl= https://web.archive.org/web/20080424093951/http://neo.jpl.nasa.gov/programs/| archivedate= 24 April 2008 <!--DASHBot-->| deadurl= nourl-status-live}}</ref>
<ref>{{cite web
| url=https://cneos.jpl.nasa.gov/stats/site_all.html
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| archive-url=https://web.archive.org/web/20181228041653/https://cneos.jpl.nasa.gov/stats/site_all.html
| archive-date=28 Desember 2018
| deadurl=nourl-status-live}}</ref>
* Lincoln Near-Earth Asteroid Research (LINEAR)
* Near-Earth Asteroid Tracking (NEAT)
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|department=Astronomy (rubriek)}}</ref> Toe sterrekundiges meer klein liggame begin vind wat permanent anderkant Jupiter bly, dit wat nou sentoure genoem word, het hulle dit as tradisionele asteroïdes beskou, hoewel gedebatteer is oor of hulle as asteroïdes beskou moet word of as ’n nuwe soort voorwerp. Toe die eerste [[trans-Neptunus-voorwerp]] (buiten [[Pluto]]), [[15760 Albion|Albion]], in 1992 ontdek word en veral toe groot getalle soortgelyke voorwerpe gevind word, is nuwe terme uitgedink om die vraagstuk te ontduik: [[Kuipergordel]]voorwerp, trans-Neptunus-voorwerp, [[Verstrooide skyf|verstrooideskyfvoorwerp]], ens. Hulle kom in die koue buitewyke van die Sonnestelsel voor waar yse [[Vaste stof|vaste stowwe]] bly en komeetagtige voorwerpe nie na verwagting veel komeetaktiwiteit toon nie; as sentoure of trans-Neptunus-voorwerpe naby die Son kom, sal hul vlugtige yse sublimeer. Hulle sal dan volgens tradisie as komete geklassifiseer word en nie as asteroïdes nie.
 
Die naaste van dié voorwerpe aan die binneste Sonnestelsel is die Kuipergordelvoorwerpe – hulle word "voorwerpe" genoem deels om ’n klassifikasie as óf komete óf asteroïdes te voorkom.<ref name=KBOasteroids>{{cite news |url=http://curious.astro.cornell.edu/question.php?number=601 |title=Are Kuiper Belt Objects asteroids? |work=Ask an astronomer |publisher=Cornell University |deadurlurl-status=yesdead |archiveurl=https://web.archive.org/web/20090103110110/http://curious.astro.cornell.edu/question.php?number=601 |archivedate=3 Januarie 2009 }}</ref> Hul samestelling is vermoedelik hoofsaaklik komeetagtig, hoewel sommige meer soos asteroïdes kan wees.<ref>{{cite web |url=http://rst.gsfc.nasa.gov/Sect19/Sect19_22.html |author=Nicholas M. Short, Sr. |title=Asteroids and Comets |website=NASA.gov |deadurlurl-status=yesdead |archiveurl=https://web.archive.org/web/20080925014037/http://rst.gsfc.nasa.gov///Sect19/Sect19_22.html|archivedate=25 September 2008}}</ref> Verder het die meeste nie die hoogs eksentrieke wentelbane wat met komete verbind word nie, en dié wat tot dusver ontdek is, is groter as tradisionele komeetkerns. (Die heelwat verder geleë [[Oortwolk]] is hipoteties die hoofbron van sluimerende komete.) Ander onlangse waarnemings, soos die ontleding van komeetstof wat deur die Stardust-sondeerder versamel is, laat toenemend die onderskeid tussen komete en asteroïdes vervaag.<ref>{{cite news |url=http://www.sciam.com/podcast/episode.cfm?id=ADD0878B-D6C3-3B70-7B5BC373545BB82D |title=Comet Dust Seems More Asteroidy |work=Scientific American |date=25 Januarie 2008}}</ref> Dit dui op ’n "onafgebrokenheid tussen asteroïdes en komete", eerder as ’n skerp skeidskyn.<ref>{{cite news |url=https://www.newscientist.com/channel/solar-system/comets-asteroids/dn13224-comet-samples-are-surprisingly-asteroidlike.html |title=Comet samples are surprisingly asteroid-like |work=New Scientist |date=24 Januarie 2008}}</ref>
 
Die kleinplanete anderkant Jupiter se wentelbaan word soms "asteroïdes" genoem. Die term word egter al hoe meer beperk tot kleinplanete in die binneste Sonnestelsel.<ref name=KBOasteroids/> In hierdie artikel word die woord se betekenis dus merendeels beperk tot die klassieke asteroïdes: voorwerpe in die [[asteroïdegordel]], [[Trojaan (sterrekunde)|Jupiter-trojane]] en [[naby-aarde-voorwerp]]e.
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| bibcode=2002AJ....123..549P |bibcode-access=free
| arxiv=astro-ph/0110258
}}</ref> as die ander asteroïdes en kan ’n laag [[ys]] op die oppervlak hê.<ref name="planetary">{{cite web|title=Asteroid 1 Ceres|work=The Planetary Society|url=http://www.planetary.org/explore/topics/asteroids_and_comets/ceres.html|accessdate=20 Oktober 2007| archiveurl= https://web.archive.org/web/20070929092440/http://planetary.org/explore/topics/asteroids_and_comets/ceres.html| archivedate= 29 September 2007 <!--DASHBot-->| deadurl= nourl-status-live}}</ref> Nes die planete is Ceres se interieur gedifferensieerd: Dit het ’n kors, ’n mantel en ’n kern.<ref name="planetary" />
 
Vesta het ook ’n gedifferensieerde interieur, maar het binne die Sonnestelsel se [[vriesgrens]] gevorm en het dus nie [[water]] nie;<ref>{{cite press release |id=STScI-1995-20 |title=Asteroid or Mini-Planet? Hubble Maps the Ancient Surface of Vesta |url=http://hubblesite.org/news_release/news/1995-20 |website=Hubble Space Telescope |date=19 April 1995 |access-date=16 Desember 2017}}<br />{{cite press release |url=http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/20/image/c |title=Key Stages in the Evolution of the Asteroid Vesta |website=Hubble Space Telescope |date=19 April 1995 |accessdate=20 Oktober 2007 |archiveurl= https://web.archive.org/web/20080907192327/http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/20/image/c| archivedate=7 September 2008<!--DASHBot-->| deadurl=nourl-status-live}}</ref><ref>{{cite journal |title=Dawn mission and operations |last1=Russel |first1=C. |last2=Raymond |first2=C. |last3=Fraschetti |first3=T. |last4=Rayman |first4=M. |last5=Polanskey |first5=C. |last6=Schimmels |first6=K. |last7=Joy |first7=S. |journal=Proceedings of the International Astronomical Union |volume=1 |issue=S229 |pages=97–119 |url=http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=414750 |date=2005 |accessdate=20 Oktober 2007 |display-authors=3 |doi=10.1017/S1743921305006691|bibcode=2006IAUS..229...97R }}</ref> hy is hoofsaaklik uit [[Lawa|basaltrots]] soos [[olivien]] saamgestel.<ref>{{cite journal |last=Burbine |first=T.H. |title=Where are the olivine asteroids in the main belt? |journal=Meteoritics |date=July 1994 |volume=29 |issue=4 |page=453 |bibcode=1994Metic..29..453B |bibcode-access=gratis}}</ref> Buiten die groot [[krater]] by sy suidpool, het Vesta ook ’n ellipsoïdale vorm. Dit is die hoofvoorwerp van die Vesta-familie en ander V-tipe asteroïdes, en is die bron van die [[Achondriet|HED-meteoriete]], wat 5% van alle [[meteoriet]]e op Aarde uitmaak.
 
Pallas is buitengewoon omdat dit, soos Uranus, op sy kant roteer, met ’n groot [[Baanhelling|hoek tussen sy rotasie-as en wentelvlak]].<ref name="Torppa1996">{{cite journal |first1=J. |last1=Torppa |first2=M. |last2=Kaasalainen |first3=T. |last3=Michałowski |first4=T. |last4=Kwiatkowski |first5=A. |last5=Kryszczyńska |first6=P. |last6=Denchev |first7=R. |last7=Kowalski
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| doi=10.1016/S0019-1035(03)00146-5 |display-authors=3}}</ref> Sy samestelling is soortgelyk aan dié van Ceres: baie [[koolstof]] en [[silikon]] en dalk gedeeltelik gedifferensieerd.<ref>{{cite journal |title=The composition of asteroid 2 Pallas and its relation to primitive meteorites |author=Larson, H.P. |author2=Feierberg, M.A. |author3=Lebofsky, L.A. |last-author-amp=yes |date=1983 |bibcode=1983Icar...56..398L |volume=56 |issue=3 |page=398 |journal=Icarus |doi=10.1016/0019-1035(83)90161-6}}</ref> Pallas is die hoofvoorwerp van die Pallas-familie asteroïdes.
 
Hygiea is die koolstofrykste asteroïde<ref>{{cite journal |title=10 Hygiea: ISO Infrared Observations |journal=Icarus |volume=156 |issue=1 |pages=202 |author=Barucci, M.A. |url=http://www.lesia.obspm.fr/~crovisier/biblio/preprint/bar02_icarus.pdf |format=PDF |date=2002 |accessdate=21 Oktober 2007 |archiveurl=https://web.archive.org/web/20071128200223/http://www.lesia.obspm.fr/~crovisier/biblio/preprint/bar02_icarus.pdf |archivedate=28 November 2007 |deadurlurl-status=yesdead |display-authors=etal |df=dmy-all|bibcode=2002Icar..156..202B |doi=10.1006/icar.2001.6775 }}</ref> en lê, anders as die ander groot asteroïdes, relatief naby aan die [[sonnebaan]].<ref>{{cite web |title=Ceres the Planet |work=orbitsimulator.com |url=http://www.orbitsimulator.com/gravity/articles/ceres.html |accessdate=20 Oktober 2007 |archiveurl=https://web.archive.org/web/20071011154140/http://orbitsimulator.com/gravity/articles/ceres.html |archivedate=11 October 2007 |deadurlurl-status=yesdead |df=dmy-all }}</ref> Dit is die grootste lid en vermoedelik die hoofvoorwerp van die Hygiea-familie asteroïdes.
 
{| class="wikitable"
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|doi=10.1007/s11208-005-0033-2
|bibcode=2005SoSyR..39..176P
|url-status=dead
|deadurl=yes
|archiveurl=https://web.archive.org/web/20140703074335/http://iau-comm4.jpl.nasa.gov/EPM2004.pdf
|archivedate=3 Julie 2014}}</ref>]]
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|publisher=The Spaceguard Foundation
|accessdate=9 April 2007
|url-status=dead
|deadurl=yes
|archiveurl=https://web.archive.org/web/20060512060350/http://spaceguard.iasf-roma.inaf.it/tumblingstone/issues/current/eng/ast-day.htm
|archivedate=12 Mei 2006
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| title=Ice confirmed on an asteroid
| publisher=Science News | url=http://www.sciencenews.org/view/generic/id/48174/title/Ice_confirmed_on_an_asteroid
| accessdate=9 Oktober 2009 | archiveurl= https://web.archive.org/web/20091012075224/http://www.sciencenews.org/view/generic/id/48174/title/Ice_confirmed_on_an_asteroid| archivedate= 12 Oktober 2009 <!--DASHBot-->| deadurl= nourl-status-live}}</ref><ref>{{cite web
| last = Atkinson
| first = Nancy
Lyn 352:
| accessdate = 11 Oktober 2009
| url = http://spacefellowship.com/2009/10/08/more-water-out-there-ice-found-on-an-asteroid/
| archiveurl= https://web.archive.org/web/20091011051040/http://spacefellowship.com/2009/10/08/more-water-out-there-ice-found-on-an-asteroid/| archivedate= 11 Oktober 2009 <!--DASHBot-->| deadurl= nourl-status-live}}</ref><ref name="Campins2010">{{ Cite journal |display-authors=3 |author1=Campins, H. |author2=Hargrove, K |author3=Pinilla-Alonso, N |author4=Howell, E.S. |author5=Kelley, M.S. |author6=Licandro, J. |author7=Mothé-Diniz, T. |author8=Fernández, Y. |author9=Ziffer, J. |title=Water ice and organics on the surface of the asteroid 24 Themis |journal=Nature |volume=464 |issue=7293 |date=2010 |doi=10.1038/nature09029 |pmid=20428164 |pages=1320–1321 |bibcode= 2010Natur.464.1320C}}</ref><ref>{{Cite journal |last=Rivkin |first=Andrew S. |last2=Emery |first2=Joshua P. |title=Detection of ice and organics on an asteroidal surface |journal=Nature |volume=464 |issue=7293 |pages=1322–1323 |date=2010 |doi=10.1038/nature09028 |pmid=20428165 |bibcode= 2010Natur.464.1322R}}</ref> Wetenskaplikes meen dit is moontlik dat van die eerste water op Aarde hierheen gebring is deur asteroïdebotsings ná die botsing wat die Maan gevorm het. Die teenwoordigheid van ys op Themis steun dié teorie.<ref name="Campins2010" />
 
In Oktober 2013 is water vir die eerste keer op ’n ekstrasolêre liggaam waargeneem – op ’n asteroïde wat om die [[witdwerg]] [[GD 61]] wentel.<ref>{{cite web |last=Mack |first=Eric |title=Newly spotted wet asteroids point to far-flung Earth-like planets |url=http://news.cnet.com/8301-17938_105-57607077-1/newly-spotted-wet-asteroids-point-to-far-flung-earth-like-planets/ |publisher=CNET}}</ref> Op 22 Januarie 2014 het wetenskaplikes van die [[Europese Ruimteagentskap]] (ESA) verslag gedoen oor die eerste besliste waarneming van [[waterdamp]] op die dwergplaneet Ceres in die asteroïdegordel.<ref name="KüppersO’Rourke2014">{{cite journal |display-authors=3 |last1=Küppers |first1=Michael |last2=O’Rourke |first2=Laurence |last3=Bockelée-Morvan |first3=Dominique |last4=Zakharov |first4=Vladimir |last5=Lee |first5=Seungwon |last6=von Allmen |first6=Paul |last7=Carry |first7=Benoît |last8=Teyssier |first8=David |last9=Marston |first9=Anthony |last10=Müller |first10=Thomas |last11=Crovisier |first11=Jacques |last12=Barucci |first12=M. Antonietta |last13=Moreno |first13=Raphael |title=Localized sources of water vapour on the dwarf planet (1) Ceres |journal=Nature |volume=505 |issue=7484 |date=2014 |pages=525–527 |doi=10.1038/nature12918 |bibcode = 2014Natur.505..525K |pmid=24451541}}</ref> Die waarneming is gedoen met die [[infrarooi]]geriewe van die [[Herschel-ruimtesterrewag]].<ref name="NASA-20140122">{{cite web |last1=Harrington |first1=J.D. |title=Herschel Telescope Detects Water on Dwarf Planet – Release 14-021 |url=http://www.nasa.gov/press/2014/january/herschel-telescope-detects-water-on-dwarf-planet |date=22 Januarie 2014 |work=NASA |accessdate=22 Januarie 2014 }}</ref> Dié bevinding was onverwags omdat komete, en nie asteroïdes nie, gewoonlik met "spuitstrale en pluime" verbind word. Volgens een van die wetenskaplikes "vervaag die verskille tussen komete en asteroïdes al hoe meer".<ref name="NASA-20140122" />
Lyn 463:
|}
 
In 1851,<ref>{{cite web| url=http://www.usno.navy.mil/USNO/astronomical-applications/astronomical-information-center/minor-planets| title=When did the asteroids become minor planets?| publisher=Naval Meteorology and Oceanography Command| accessdate=6 November 2011| deadurlurl-status=yesdead| archiveurl=https://web.archive.org/web/20120406222551/http://www.usno.navy.mil/USNO/astronomical-applications/astronomical-information-center/minor-planets/| archivedate=6 April 2012| df=dmy-all}}</ref> nadat die 15de asteroïde (15 Eunomia) ontdek is, het [[Johann Franz Encke]] ’n groot verandering aangebring aan die komende 1854-uitgawe van die ''Berliner Astronomisches Jahrbuch'' (BAJ, "Berlynse Astronomiese Jaarboek"). Hy het ’n skyf (sirkel), tradisioneel die simbool vir ’n ster, as ’n generiese simbool vir ’n asteroïde begin gebruik. Die sirkel is toe genommer in die volgorde van ontdekking om ’n spesifieke asteroïde aan te dui (hoewel hy <big>①</big> aan die vyfde asteroïde, 5 Astraea, toegeken het) – vir die eerste vier het hy slegs hul bestaande ikoniese simbole gebruik. Sterrekundiges het gou dié metode gevolg, en die volgende asteroïde wat ontdek is (16 Psyche, in 1852) was die eerste een wat met sy ontdekking volgens sy nommer aangedui is. Psyche en ’n paar ander het egter ook ikoniese simbole gekry. 20 Massalia was die eerste een wat nie ’n ikoniese simbool gekry het nie, en ná die ontdekking in 1855 van 37 Fides is geen ikoniese simbole meer toegeken nie. Astraea se nommer is in dié jaar na <big>⑤</big> geskuif, maar die eerste vier asteroïdes is eers van die 1867-uitgawe af volgens hul nommers aangedui. Die sirkel is daarna in hakies verander, wat makliker was om te druk, en oor die volgende paar dekades soms weggelaat. Dit het tot die huidige gebruik aanleiding gegee.<ref name="hilton"/>
 
==Verkenning==