233:
275:, with a series of concentric peak rings that enclose a central depression. Burney's degraded state makes it difficult to discern its extent due to the subtle nature of its peak rings; Burney may have anywhere from 2–4 such rings. As such, estimates for Burney's diameter range from ~290 kilometers to ~350 kilometers. The peak rings of Burney are discontinuous and crenulated, standing roughly 500–1,000 meters high. The central depression of Burney is approximately 180 kilometers across and roughly 1.8–3 kilometers deep. Within Burney are numerous smaller impact craters, one of which has been officially named
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1227:
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29:
251:
302:. This terrain is characterized by parallel ridges spaced 1–2 kilometers apart and covers large parts of Burney's basin floor. One hypothesis for the origin of the washboard terrain is from the collection and deposition of material from an ancient period of heavy regional glaciation. The age of the washboard terrain appears to only marginally postdate the
350:, a similarly-sized crater on the anti-encounter hemisphere of Pluto, may have multiple rings. Sputnik Planitia basin, though much larger, does not have visible rings; any internal structural features are buried beneath its nitrogen glaciers. The blocky mountains alongside Sputnik Planitia's western border may be related to a peak ring within the basin.
290:
ice, indicating that methane preferentially condenses on the high-altitude mountain peaks that comprise Burney's concentric rings. By contrast, Burney's floor is poor in methane ice and much smoother than the surrounding plains, possibly from differences in erosion or from heavier glaciation. Several
242:
image of a section of Burney and its interior craters. One of Burney's rings form a chain of mountains that arcs across the image. Scale bar of 6 mi (9.7 km) is at the top left
778:
Schmitt, B.; Philippe, S.; Grundy, W. M.; et al. (May 2017). "Physical state and distribution of materials at the surface of Pluto from New
Horizons LEISA imaging spectrometer".
39:
of Burney basin, center. An ancient impact basin, its heavily eroded state makes it difficult to discern; its concentric rings are only slightly brighter than the surrounding plains
550:
Moruzzi, Samantha A.; Andrews-Hanna, Jeffrey C.; Schenk, Paul; Johnson, Brandon C. (November 2023). "Pluto's
Sputnik basin as a peak-ring or multiring basin: A comparative study".
291:
dark streaks similar to those found in
Sputnik Planitia were observed in and around Burney. Models of Pluto's climate indicate that Burney likely experiences downward-flowing
898:
655:
White, Oliver L.; Moore, Jeffrey M.; Howard, Alan D.; et al. (January 2019). "Washboard and fluted terrains on Pluto as evidence for ancient glaciation".
162:. With a diameter of over 290 kilometers and possibly up to 350 kilometers, it is the second-largest known impact basin on Pluto, after the
72:
267:. It is ancient, with an estimated age of at least 4 billion years old, and heavily eroded. The structure of Burney resembles that of the
468:
Stern, S. Alan; Keeney, Brian; Hoover, Rachael; Protopapa, Silvia; White, Oliver; Grundy, William; Cruikshank, Dale P. (November 2021).
813:
Hofgartner, J. D.; Buratti, B. J.; Devins, S. L.; et al. (March 2018). "A search for temporal changes on Pluto and Charon".
298:
Surrounding Burney basin is a broad region to the northwest of
Sputnik Planitia that hosts a type of terrain informally called
606:
256:
A topography map of Burney, where its Mare
Orientale-style degraded peak rings and central depression are much more apparent
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Burney is the second-largest impact feature known on Pluto, after the massive basin that encloses the glacial plains of
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443:
Stern, S. Alan (August 2021). Moore, Jeffrey M.; Grundy, William M.; Young, Leslie A.; Binzel, Richard P. (eds.).
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basin. Burney is the only impact basin with visible multiple rings known on Pluto and is thus classified as a
1003:
698:
529:
Viscous relaxation of Oort and
Edgeworth craters on Pluto: Possible indication of early high heat flows
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729:"Pluto's Surface Mapping Using Unsupervised Learning from Near-infrared Observations of LEISA/Ralph"
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Forget, F.; Bertrand, T.; Vangvichith, M.; Leconte, J.; Millour, E.; Lellouch, E. (May 2017).
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470:"New Investigations of Dark-floored Pits In the Volatile Ice of Sputnik Planitia on Pluto"
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413:. 48th Lunar and Planetary Science Conference. The Woodlands, Texas, United States. 2854
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860:"A post-new horizons global climate model of Pluto including the N2, CH4 and CO cycles"
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727:; Ahrens, C. J.; Khan, M. K. H.; Chevrier, V. F.; Cruikshank, D. P. (January 2023).
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Much of Burney basin is glaciated, its surface covered in bright, coarse grains of
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318: – Lunar mare on the western border of the near side and far side of the Moon
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McKinnon, William; Singer, Kelsi; Robbins, Stuart; et al. (December 2023).
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630:"Relative and Absolute Ages of Pluto and Charon's Surfaces Using Crater Counts"
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387:(Center Latitude: 45.68°, Center Longitude: 133.79°; Planetocentric, +East)
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As with the rest of Pluto's surface features, Burney was first seen on the
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mixed with water ice. The peak rings of Burney are additionally coated in
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McKinnon, William B.; Schenk, P. M.; Mao, X.; et al. (March 2017).
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704:. Gazetteer of Planetary Nomeclature. 22 September 2023
195:
on 14 July 2015. The impact basin was informally named
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531:. AAS Division of Planetary Science meeting #54.
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215:in 1930. The name was officially approved by the
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407:Impact Origin of Sputnik Planitia Basin, Pluto
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324: – Lunar mare on the far side of the Moon
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385:. USGS Astrogeology Research Program.
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628:Gosmeyer, C. M. (16 December 2015).
609:from the original on 4 October 2018
447:. The University of Arizona Press.
445:The Pluto System After New Horizons
383:Gazetteer of Planetary Nomenclature
13:
364:
14:
1486:
211:to the dwarf planet's discoverer
107:296–350 km (184–217 mi)
1225:
1219:
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599:Pluto: The Discovery of Planet X
593:Rincon, Paul (13 January 2006).
330: – Largest crater on Charon
249:
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217:International Astronomical Union
115:~1.8–3 km (1.1–1.9 mi)
16:Multi-ring impact basin on Pluto
147:, sometimes referred to as the
341:
151:, is the second-largest known
1:
733:The Planetary Science Journal
595:"The girl who named a planet"
357:
887:10.1016/j.icarus.2016.11.038
845:10.1016/j.icarus.2017.10.044
800:10.1016/j.icarus.2016.12.025
572:10.1016/j.icarus.2023.115721
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1475:Discoveries by New Horizons
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677:10.1038/s41550-018-0592-z
207:, who suggested the name
168:multi-ringed impact basin
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1314:IAU definition of planet
505:10.3847/1538-3881/ac24a6
474:The Astronomical Journal
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219:(IAU) on 8 August 2017.
48:Multi-ring impact basin
1414:Trans-Neptunian object
1115:Coleta de Dados Colles
322:Mare Moscoviense basin
306:that created Burney.
1309:Definition of planet
1302:Official definitions
1072:Tombaugh "The Heart"
699:"Pluto Nomenclature"
316:Mare Orientale basin
174:Discovery and naming
1340:Neil deGrasse Tyson
879:2017Icar..287...54F
837:2018Icar..302..273H
792:2017Icar..287..229S
755:2023PSJ.....4...15E
669:2019NatAs...3...62W
564:2023Icar..40515721M
537:2022DPS....5430303M
496:2021AJ....162..207S
84: /
23:
1361:Lowell Observatory
1323:Scientist opinions
764:10.3847/PSJ/acb0cc
238:A high-resolution
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1110:Challenger Colles
300:washboard terrain
203:team in honor of
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1399:Dwarf planet
1376:Roger Putnam
1285:New Horizons
1283:
1243:
1200:
1125:Piccard Mons
1105:Baret Montes
906:. Retrieved
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415:. Retrieved
406:
382:
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304:impact event
299:
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284:nitrogen ice
281:
276:
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240:New Horizons
239:
201:New Horizons
200:
196:
181:New Horizons
179:
177:
157:dwarf planet
153:impact basin
149:Burney basin
148:
144:
143:
125:New Horizons
123:
57:Venera Terra
45:Feature type
36:New Horizons
34:
18:
1419:Kuiper belt
1276:Exploration
1162:depressions
1160:Valleys and
1135:Wright Mons
821:: 273–284.
786:: 229–260.
723:Emran, A.;
138:(1918–2009)
91: /
67:Coordinates
1464:Categories
1330:Alan Stern
1185:Luna Linea
1025:Vucub-Came
1020:Harrington
962:Atmosphere
828:1711.02750
746:2301.06027
487:2109.01025
480:(5): 207.
358:References
193:five moons
120:Discoverer
1444:Mythology
1349:Discovery
1295:Astronomy
1098:mountains
1096:Hills and
982:Geography
895:125136232
873:: 54–71.
739:(1): 15.
685:135139421
663:: 62–68.
582:. 115721.
580:260217921
539:. 303.03.
514:237385294
348:Simonelli
1356:Planet X
1256:Kerberos
1052:Hayabusa
1030:Hun-Came
1010:Safronov
987:features
899:Archived
613:12 April
607:Archived
603:BBC News
379:"Burney"
310:See also
277:Hardaway
191:and its
104:Diameter
79:133°47′E
53:Location
1439:Fiction
1432:Related
1409:Plutino
1387:General
1194:Craters
1087:Voyager
1067:Pioneer
1062:Morgoth
996:Regions
972:Geology
967:Climate
875:Bibcode
833:Bibcode
788:Bibcode
751:Bibcode
665:Bibcode
560:Bibcode
533:Bibcode
492:Bibcode
328:Dorothy
288:methane
223:Geology
199:by the
155:on the
76:45°41′N
1404:Planet
1245:Charon
1201:Burney
1178:Lineae
1144:Plains
1082:Viking
1077:Venera
1057:Lowell
1047:Cadejo
1042:Belton
1015:Sharaf
893:
867:Icarus
815:Icarus
780:Icarus
683:
578:
552:Icarus
516:. 207.
512:
451:
197:Burney
145:Burney
132:Eponym
22:Burney
1251:Hydra
1236:Moons
951:Pluto
908:4 May
902:(PDF)
891:S2CID
863:(PDF)
823:arXiv
767:. 54.
741:arXiv
708:4 May
702:(PDF)
681:S2CID
635:4 May
576:S2CID
510:S2CID
482:arXiv
417:4 May
411:(PDF)
335:Notes
209:Pluto
189:Pluto
185:flyby
160:Pluto
112:Depth
61:Pluto
1266:Styx
910:2024
710:2024
637:2024
615:2007
449:ISBN
419:2024
273:Moon
1261:Nix
883:doi
871:287
841:doi
819:302
796:doi
784:287
759:doi
673:doi
568:doi
556:405
500:doi
478:162
187:of
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