English: This image shows Caravaggio, a double-ring impact basin (approximately 160 kilometers in diameter), with another large impact crater on its south-south-western side. Smaller, more recent impacts formed comparatively fresh craters across the entire surface visible in this image. The floor within the inner or peak ring appears to be smoother than the floor between the peak ring and the outer rim, possibly the result of lava flows that partially flooded the basin some time after impact. Double-ring basins are formed when a large meteoroid strikes the surface of a rocky planet. Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS). ID: EN0162744214M. Acquired: Third flyby on 2009-09-29. Resolution: 400 meters/pixel. Scale: The double-ring basin is approximately 160 kilometres in diameter. Spacecraft Altitude: 15,400 kilometres.
วันที่
แหล่งที่มา
MESSENGER
ผู้สร้างสรรค์
NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
{{Information |Description={{en|1=This image shows a double-ring impact basin, with another large impact crater on its south-south-western side. Smaller, more recent impacts formed comparatively fresh craters across the entire surface visible in this imag
ไฟล, mercury, double, ring, impact, basin, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลางขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, โลไบต, ชน, ดไมม, image, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย, คอมมอน. ifl prawtiifl hnathimiphaphni karichiflswnklangkhnadkhxngtwxyangni 596 600 phikesl khwamlaexiydxun 239 240 phikesl 477 480 phikesl 1 018 1 024 phikesl duphaphthimikhwamlaexiydsungkwa 8206 1 018 1 024 phikesl khnadifl 771 kiolibt chnidimm image png rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibayMercury Double Ring Impact Basin png English This image shows Caravaggio a double ring impact basin approximately 160 kilometers in diameter with another large impact crater on its south south western side Smaller more recent impacts formed comparatively fresh craters across the entire surface visible in this image The floor within the inner or peak ring appears to be smoother than the floor between the peak ring and the outer rim possibly the result of lava flows that partially flooded the basin some time after impact Double ring basins are formed when a large meteoroid strikes the surface of a rocky planet Instrument Narrow Angle Camera NAC of the Mercury Dual Imaging System MDIS ID EN0162744214M Acquired Third flyby on 2009 09 29 Resolution 400 meters pixel Scale The double ring basin is approximately 160 kilometres in diameter Spacecraft Altitude 15 400 kilometres wnthi 7 tulakhm ph s 2552 aehlngthima MESSENGER phusrangsrrkh NASA Johns Hopkins University Applied Physics Laboratory Carnegie Institution of Washington karxnuyatichsiththi Public domain Public domain false false phaphniepnsatharnsmbti enuxngcakepnphaphthisrangkhunodyxngkhkarbriharkarbinaelaxwkasaehngchati NASA sungtamnoybaydanlikhsiththikhxngnasarabuiwwa phaphaelasuxtang khxngnasaimidrbkarkhumkhrxngodylikhsiththiykewncarabuiwwamilikhsiththi duephimthi hnanoybaydanlikhsiththikhxngnasa hrux noybaykarichphaphkhxng JPL khaetuxn karich olokkhxngnasa ekhruxnghmayaelaekhruxngpradbkhxngnasa thukcakddwykdhmayshrthxemrikainlksna 14 khxngkhxbngkhbthangrachkarshrthxemrika swnthi 1221 ewbistkhxngnasaekbrwbrwmphaphthimacakxngkhkarxwkasosewiyt xngkhkarxwkasaehngchatirsesiy aelaxngkhkarxwkasthimiichxngkhkarxwkaskhxngshrthxemrika epncanwnmak phaphehlaniimcaepntxngepnsatharnsmbtiesmxip phaphhruxsuxthimacak klxngothrthrrsnxwkashbebil xacmilikhsiththi hakphaphhruxsuxnnimidrabuchdecnwamacak sthabnwithyasastrklxngothrthrrsnxwkas 1 phaphhruxsuxthnghmdthimacakekhruxngmuxkhxng okhrngkarsuksadwngxathityaelalmsuriya milikhsiththi karnaphaphhruxsuxcakokhrngkaripichnxkehnuxcakkarichephuxkarkhahruxephuxkarsuksa txngidrbxnuyatkxn 2 phaphthithukkhdeluxkihepn phaphdarasastrpracawn APOD bnewbistkhxng APOD xacmilikhsiththi 3 khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairixethmthiaesdngxyuiniflniprakxbdwywnthisrang wnkxtng7 tulakhm 2009MIME type nbsp xngkvsimage png prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn16 04 7 tulakhm 25521 018 1 024 771 kiolibt Originalwana Information Description en 1 This image shows a double ring impact basin with another large impact crater on its south south western side Smaller more recent impacts formed comparatively fresh craters across the entire surface visible in this imag hnathimiphaphni hnatxipni oyngmathiphaphni dawphuth karichiflswnklang wikixuntxipniichiflni karichbn en wikipedia org Geology of Mercury Caravaggio crater karichbn en wikiversity org User Marshallsumter Keynote lectures draft Mercury Draft Original research Astrogeology Astronomy college course Mercury User Marshallsumter Radiation astronomy1 Minerals User Marshallsumter Rocks Rocky objects Mercury Liquids Liquid objects Mercury karichbn eu wikipedia org Bonbardaketa Berantiar Handia karichbn fr wikipedia org Geologie de Mercure karichbn ja wikipedia org 水星の地質 karichbn ko wikipedia org 수성의 지질학 karichbn mk wikipedia org Geologiјa na Merkur karichbn sk wikipedia org Portal Astronomia Obrazky tyzdna 2013 Portal Astronomia Obrazok tyzdna 7 2013 karichbn uk wikipedia org Merkurij planeta karichbn vi wikipedia org Địa chất Sao Thủy karichbn zh wikipedia org 水星地質 ekhathungcak https th wikipedia org wiki ifl Mercury Double Ring Impact Basin png, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
