The trans-neptunian object UB313 is larger than Pluto

One over the nine The discovery of the trans-neptunian object 2003 UB 313 in July 2005 has rekindled the debate over which objects should be called planets. Popularly but not officially known as the ‘tenth planet’, its optical brightness suggests it is larger than Pluto, but without knowing its surf...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Nature 2006-02, Vol.439 (7076), p.563-564
Hauptverfasser: Bertoldi, F., Altenhoff, W., Weiss, A., Menten, K.M., Thum, C.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 564
container_issue 7076
container_start_page 563
container_title Nature
container_volume 439
creator Bertoldi, F.
Altenhoff, W.
Weiss, A.
Menten, K.M.
Thum, C.
description One over the nine The discovery of the trans-neptunian object 2003 UB 313 in July 2005 has rekindled the debate over which objects should be called planets. Popularly but not officially known as the ‘tenth planet’, its optical brightness suggests it is larger than Pluto, but without knowing its surface reflectivity (albedo) it is not possible to determine size from optical data. But now a pretty accurate measure of its size has be made, based on thermal emission data obtained using the IRAM 30-metre radio telescope at Pico Veleta, Spain. UB 313 is about 3,000 km in diameter, compared to Pluto's 2,000 km. Its albedo is similar to Pluto's, consistent with a highly reflective icy surface rich in methane. The most distant known object in the Solar System, 2003 UB 313 (97  au from the Sun), was recently discovered near its aphelion 1 . Its high eccentricity and inclination to the ecliptic plane, along with its perihelion near the orbit of Neptune, identify it as a member of the ‘scattered disk’. This disk of bodies probably originates in the Kuiper belt objects, which orbit near the ecliptic plane in circular orbits between 30 and 50  au , and may include Pluto as a member. The optical brightness of 2003 UB 313 , if adjusted to Pluto's distance, is greater than that of Pluto, which suggested that it might be larger than Pluto 2 . The actual size, however, could not be determined from the optical measurements because the surface reflectivity (albedo) was unknown. Here we report observations of the thermal emission of 2003 UB 313 at a wavelength of 1.2 mm, which in combination with the measured optical brightness leads to a diameter of 3,000 ± 300 ± 100 km. Here the first error reflects measurement uncertainties, while the second derives from the unknown object orientation. This makes 2003 UB 313 the largest known trans-neptunian object, even larger than Pluto (2,300 km) 3 . The albedo is 0.60 ± 0.10 ± 0.05, which is strikingly similar to that of Pluto, suggesting that the methane seen in the optical spectrum 2 causes a highly reflective icy surface.
doi_str_mv 10.1038/nature04494
format Article
fullrecord <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_miscellaneous_743521114</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A185465691</galeid><sourcerecordid>A185465691</sourcerecordid><originalsourceid>FETCH-LOGICAL-c649t-5e3f7f98915755553c67da6ac4ed3b0d564d204d5012a1335929596f277dd6b83</originalsourceid><addsrcrecordid>eNqN0luL00AYBuBBFLeuXnkvQVARzTrnw2UtHhYWFe3i5TCdfOlmSSfdmQnov3dKC91KPWQuApknX5g3L0KPCT4jmOk3weUxAubc8DtoQriSNZda3UUTjKmusWbyBD1I6RpjLIji99EJkVxQo9gEifkVVDm6kOoA6zyGzoVqWFyDz9XlW0ZY1aWqd3EJscpXZe9LP-bhIbrXuj7Bo939FF2-fzeffawvPn84n00vai-5ybUA1qrWaEOEEuViXqrGSec5NGyBGyF5QzFvBCbUEcaEoUYY2VKlmkYuNDtFL7Zz13G4GSFlu-qSh753AYYxWcWZoIQQXuTzv0qpJGVa6n9CarBSjP8H1NgYKUyBT3-D18MYQ8nFlsMJLpTeTKu3aOl6sF1ohxK6X0KA6PohQNuVx1OiBZdCGrIfeuD9uruxt9HZEVRWA6vOH5368uCFYjL8yEs3pmTPv309tK_-bKfz77NPR7WPQ0oRWruO3crFn5Zgu6mpvVXTop_sIhsXK2j2dtfLAp7tgEve9W0pqO_S3pUfzyneZP9661LZCqWk--yPffcXAf73Xw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>204545788</pqid></control><display><type>article</type><title>The trans-neptunian object UB313 is larger than Pluto</title><source>Nature</source><source>Alma/SFX Local Collection</source><creator>Bertoldi, F. ; Altenhoff, W. ; Weiss, A. ; Menten, K.M. ; Thum, C.</creator><creatorcontrib>Bertoldi, F. ; Altenhoff, W. ; Weiss, A. ; Menten, K.M. ; Thum, C.</creatorcontrib><description>One over the nine The discovery of the trans-neptunian object 2003 UB 313 in July 2005 has rekindled the debate over which objects should be called planets. Popularly but not officially known as the ‘tenth planet’, its optical brightness suggests it is larger than Pluto, but without knowing its surface reflectivity (albedo) it is not possible to determine size from optical data. But now a pretty accurate measure of its size has be made, based on thermal emission data obtained using the IRAM 30-metre radio telescope at Pico Veleta, Spain. UB 313 is about 3,000 km in diameter, compared to Pluto's 2,000 km. Its albedo is similar to Pluto's, consistent with a highly reflective icy surface rich in methane. The most distant known object in the Solar System, 2003 UB 313 (97  au from the Sun), was recently discovered near its aphelion 1 . Its high eccentricity and inclination to the ecliptic plane, along with its perihelion near the orbit of Neptune, identify it as a member of the ‘scattered disk’. This disk of bodies probably originates in the Kuiper belt objects, which orbit near the ecliptic plane in circular orbits between 30 and 50  au , and may include Pluto as a member. The optical brightness of 2003 UB 313 , if adjusted to Pluto's distance, is greater than that of Pluto, which suggested that it might be larger than Pluto 2 . The actual size, however, could not be determined from the optical measurements because the surface reflectivity (albedo) was unknown. Here we report observations of the thermal emission of 2003 UB 313 at a wavelength of 1.2 mm, which in combination with the measured optical brightness leads to a diameter of 3,000 ± 300 ± 100 km. Here the first error reflects measurement uncertainties, while the second derives from the unknown object orientation. This makes 2003 UB 313 the largest known trans-neptunian object, even larger than Pluto (2,300 km) 3 . The albedo is 0.60 ± 0.10 ± 0.05, which is strikingly similar to that of Pluto, suggesting that the methane seen in the optical spectrum 2 causes a highly reflective icy surface.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>EISSN: 1476-4679</identifier><identifier>DOI: 10.1038/nature04494</identifier><identifier>PMID: 16452973</identifier><identifier>CODEN: NATUAS</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Albedo ; Astronomy ; Earth, ocean, space ; Emissions ; Exact sciences and technology ; Humanities and Social Sciences ; Interplanetary space ; Kuiper belt ; letter ; Methane ; multidisciplinary ; Orbits ; Science ; Science (multidisciplinary) ; Solar system ; Stars &amp; galaxies</subject><ispartof>Nature, 2006-02, Vol.439 (7076), p.563-564</ispartof><rights>Springer Nature Limited 2006</rights><rights>2006 INIST-CNRS</rights><rights>COPYRIGHT 2006 Nature Publishing Group</rights><rights>Copyright Nature Publishing Group Feb 2, 2006</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c649t-5e3f7f98915755553c67da6ac4ed3b0d564d204d5012a1335929596f277dd6b83</citedby><cites>FETCH-LOGICAL-c649t-5e3f7f98915755553c67da6ac4ed3b0d564d204d5012a1335929596f277dd6b83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=17434209$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/16452973$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Bertoldi, F.</creatorcontrib><creatorcontrib>Altenhoff, W.</creatorcontrib><creatorcontrib>Weiss, A.</creatorcontrib><creatorcontrib>Menten, K.M.</creatorcontrib><creatorcontrib>Thum, C.</creatorcontrib><title>The trans-neptunian object UB313 is larger than Pluto</title><title>Nature</title><addtitle>Nature</addtitle><addtitle>Nature</addtitle><description>One over the nine The discovery of the trans-neptunian object 2003 UB 313 in July 2005 has rekindled the debate over which objects should be called planets. Popularly but not officially known as the ‘tenth planet’, its optical brightness suggests it is larger than Pluto, but without knowing its surface reflectivity (albedo) it is not possible to determine size from optical data. But now a pretty accurate measure of its size has be made, based on thermal emission data obtained using the IRAM 30-metre radio telescope at Pico Veleta, Spain. UB 313 is about 3,000 km in diameter, compared to Pluto's 2,000 km. Its albedo is similar to Pluto's, consistent with a highly reflective icy surface rich in methane. The most distant known object in the Solar System, 2003 UB 313 (97  au from the Sun), was recently discovered near its aphelion 1 . Its high eccentricity and inclination to the ecliptic plane, along with its perihelion near the orbit of Neptune, identify it as a member of the ‘scattered disk’. This disk of bodies probably originates in the Kuiper belt objects, which orbit near the ecliptic plane in circular orbits between 30 and 50  au , and may include Pluto as a member. The optical brightness of 2003 UB 313 , if adjusted to Pluto's distance, is greater than that of Pluto, which suggested that it might be larger than Pluto 2 . The actual size, however, could not be determined from the optical measurements because the surface reflectivity (albedo) was unknown. Here we report observations of the thermal emission of 2003 UB 313 at a wavelength of 1.2 mm, which in combination with the measured optical brightness leads to a diameter of 3,000 ± 300 ± 100 km. Here the first error reflects measurement uncertainties, while the second derives from the unknown object orientation. This makes 2003 UB 313 the largest known trans-neptunian object, even larger than Pluto (2,300 km) 3 . The albedo is 0.60 ± 0.10 ± 0.05, which is strikingly similar to that of Pluto, suggesting that the methane seen in the optical spectrum 2 causes a highly reflective icy surface.</description><subject>Albedo</subject><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Emissions</subject><subject>Exact sciences and technology</subject><subject>Humanities and Social Sciences</subject><subject>Interplanetary space</subject><subject>Kuiper belt</subject><subject>letter</subject><subject>Methane</subject><subject>multidisciplinary</subject><subject>Orbits</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>Solar system</subject><subject>Stars &amp; galaxies</subject><issn>0028-0836</issn><issn>1476-4687</issn><issn>1476-4679</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNqN0luL00AYBuBBFLeuXnkvQVARzTrnw2UtHhYWFe3i5TCdfOlmSSfdmQnov3dKC91KPWQuApknX5g3L0KPCT4jmOk3weUxAubc8DtoQriSNZda3UUTjKmusWbyBD1I6RpjLIji99EJkVxQo9gEifkVVDm6kOoA6zyGzoVqWFyDz9XlW0ZY1aWqd3EJscpXZe9LP-bhIbrXuj7Bo939FF2-fzeffawvPn84n00vai-5ybUA1qrWaEOEEuViXqrGSec5NGyBGyF5QzFvBCbUEcaEoUYY2VKlmkYuNDtFL7Zz13G4GSFlu-qSh753AYYxWcWZoIQQXuTzv0qpJGVa6n9CarBSjP8H1NgYKUyBT3-D18MYQ8nFlsMJLpTeTKu3aOl6sF1ohxK6X0KA6PohQNuVx1OiBZdCGrIfeuD9uruxt9HZEVRWA6vOH5368uCFYjL8yEs3pmTPv309tK_-bKfz77NPR7WPQ0oRWruO3crFn5Zgu6mpvVXTop_sIhsXK2j2dtfLAp7tgEve9W0pqO_S3pUfzyneZP9661LZCqWk--yPffcXAf73Xw</recordid><startdate>20060202</startdate><enddate>20060202</enddate><creator>Bertoldi, F.</creator><creator>Altenhoff, W.</creator><creator>Weiss, A.</creator><creator>Menten, K.M.</creator><creator>Thum, C.</creator><general>Nature Publishing Group UK</general><general>Nature Publishing</general><general>Nature Publishing Group</general><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>ATWCN</scope><scope>3V.</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QR</scope><scope>7RV</scope><scope>7SN</scope><scope>7SS</scope><scope>7ST</scope><scope>7T5</scope><scope>7TG</scope><scope>7TK</scope><scope>7TM</scope><scope>7TO</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88E</scope><scope>88G</scope><scope>88I</scope><scope>8AF</scope><scope>8AO</scope><scope>8C1</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>D1I</scope><scope>DWQXO</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H94</scope><scope>HCIFZ</scope><scope>K9.</scope><scope>KB.</scope><scope>KB0</scope><scope>KL.</scope><scope>L6V</scope><scope>LK8</scope><scope>M0K</scope><scope>M0S</scope><scope>M1P</scope><scope>M2M</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>NAPCQ</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PSYQQ</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>S0X</scope><scope>SOI</scope><scope>7U5</scope><scope>L7M</scope><scope>H8D</scope><scope>7X8</scope><scope>7SC</scope><scope>7SP</scope><scope>7SR</scope><scope>7TB</scope><scope>8BQ</scope><scope>F28</scope><scope>JG9</scope><scope>JQ2</scope><scope>KR7</scope><scope>L~C</scope><scope>L~D</scope></search><sort><creationdate>20060202</creationdate><title>The trans-neptunian object UB313 is larger than Pluto</title><author>Bertoldi, F. ; Altenhoff, W. ; Weiss, A. ; Menten, K.M. ; Thum, C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c649t-5e3f7f98915755553c67da6ac4ed3b0d564d204d5012a1335929596f277dd6b83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Albedo</topic><topic>Astronomy</topic><topic>Earth, ocean, space</topic><topic>Emissions</topic><topic>Exact sciences and technology</topic><topic>Humanities and Social Sciences</topic><topic>Interplanetary space</topic><topic>Kuiper belt</topic><topic>letter</topic><topic>Methane</topic><topic>multidisciplinary</topic><topic>Orbits</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>Solar system</topic><topic>Stars &amp; galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bertoldi, F.</creatorcontrib><creatorcontrib>Altenhoff, W.</creatorcontrib><creatorcontrib>Weiss, A.</creatorcontrib><creatorcontrib>Menten, K.M.</creatorcontrib><creatorcontrib>Thum, C.</creatorcontrib><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Gale In Context: Middle School</collection><collection>ProQuest Central (Corporate)</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium &amp; Calcified Tissue Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Nursing &amp; Allied Health Database</collection><collection>Ecology Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Environment Abstracts</collection><collection>Immunology Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Oncogenes and Growth Factors Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>Agricultural Science Collection</collection><collection>Health &amp; Medical Collection</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Psychology Database (Alumni)</collection><collection>Science Database (Alumni Edition)</collection><collection>STEM Database</collection><collection>ProQuest Pharma Collection</collection><collection>Public Health Database</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>Agricultural &amp; Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>eLibrary</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central Korea</collection><collection>Engineering Research Database</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Health &amp; Medical Complete (Alumni)</collection><collection>Materials Science Database</collection><collection>Nursing &amp; Allied Health Database (Alumni Edition)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>ProQuest Engineering Collection</collection><collection>ProQuest Biological Science Collection</collection><collection>Agricultural Science Database</collection><collection>Health &amp; Medical Collection (Alumni Edition)</collection><collection>Medical Database</collection><collection>Psychology Database</collection><collection>Research Library</collection><collection>Science Database</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>Biological Science Database</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>Nursing &amp; Allied Health Premium</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>Materials Science Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest One Psychology</collection><collection>Engineering Collection</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>University of Michigan</collection><collection>Genetics Abstracts</collection><collection>SIRS Editorial</collection><collection>Environment Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Aerospace Database</collection><collection>MEDLINE - Academic</collection><collection>Computer and Information Systems Abstracts</collection><collection>Electronics &amp; Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Mechanical &amp; Transportation Engineering Abstracts</collection><collection>METADEX</collection><collection>ANTE: Abstracts in New Technology &amp; Engineering</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Civil Engineering Abstracts</collection><collection>Computer and Information Systems Abstracts – Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><jtitle>Nature</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bertoldi, F.</au><au>Altenhoff, W.</au><au>Weiss, A.</au><au>Menten, K.M.</au><au>Thum, C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The trans-neptunian object UB313 is larger than Pluto</atitle><jtitle>Nature</jtitle><stitle>Nature</stitle><addtitle>Nature</addtitle><date>2006-02-02</date><risdate>2006</risdate><volume>439</volume><issue>7076</issue><spage>563</spage><epage>564</epage><pages>563-564</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><eissn>1476-4679</eissn><coden>NATUAS</coden><abstract>One over the nine The discovery of the trans-neptunian object 2003 UB 313 in July 2005 has rekindled the debate over which objects should be called planets. Popularly but not officially known as the ‘tenth planet’, its optical brightness suggests it is larger than Pluto, but without knowing its surface reflectivity (albedo) it is not possible to determine size from optical data. But now a pretty accurate measure of its size has be made, based on thermal emission data obtained using the IRAM 30-metre radio telescope at Pico Veleta, Spain. UB 313 is about 3,000 km in diameter, compared to Pluto's 2,000 km. Its albedo is similar to Pluto's, consistent with a highly reflective icy surface rich in methane. The most distant known object in the Solar System, 2003 UB 313 (97  au from the Sun), was recently discovered near its aphelion 1 . Its high eccentricity and inclination to the ecliptic plane, along with its perihelion near the orbit of Neptune, identify it as a member of the ‘scattered disk’. This disk of bodies probably originates in the Kuiper belt objects, which orbit near the ecliptic plane in circular orbits between 30 and 50  au , and may include Pluto as a member. The optical brightness of 2003 UB 313 , if adjusted to Pluto's distance, is greater than that of Pluto, which suggested that it might be larger than Pluto 2 . The actual size, however, could not be determined from the optical measurements because the surface reflectivity (albedo) was unknown. Here we report observations of the thermal emission of 2003 UB 313 at a wavelength of 1.2 mm, which in combination with the measured optical brightness leads to a diameter of 3,000 ± 300 ± 100 km. Here the first error reflects measurement uncertainties, while the second derives from the unknown object orientation. This makes 2003 UB 313 the largest known trans-neptunian object, even larger than Pluto (2,300 km) 3 . The albedo is 0.60 ± 0.10 ± 0.05, which is strikingly similar to that of Pluto, suggesting that the methane seen in the optical spectrum 2 causes a highly reflective icy surface.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>16452973</pmid><doi>10.1038/nature04494</doi><tpages>2</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0028-0836
ispartof Nature, 2006-02, Vol.439 (7076), p.563-564
issn 0028-0836
1476-4687
1476-4679
language eng
recordid cdi_proquest_miscellaneous_743521114
source Nature; Alma/SFX Local Collection
subjects Albedo
Astronomy
Earth, ocean, space
Emissions
Exact sciences and technology
Humanities and Social Sciences
Interplanetary space
Kuiper belt
letter
Methane
multidisciplinary
Orbits
Science
Science (multidisciplinary)
Solar system
Stars & galaxies
title The trans-neptunian object UB313 is larger than Pluto
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-19T05%3A56%3A53IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20trans-neptunian%20object%20UB313%20is%20larger%20than%20Pluto&rft.jtitle=Nature&rft.au=Bertoldi,%20F.&rft.date=2006-02-02&rft.volume=439&rft.issue=7076&rft.spage=563&rft.epage=564&rft.pages=563-564&rft.issn=0028-0836&rft.eissn=1476-4687&rft.coden=NATUAS&rft_id=info:doi/10.1038/nature04494&rft_dat=%3Cgale_proqu%3EA185465691%3C/gale_proqu%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=204545788&rft_id=info:pmid/16452973&rft_galeid=A185465691&rfr_iscdi=true