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İzahMoon Farside LRO.jpg
English: Far side of the moon, by NASA's Lunar Reconnaissance Orbiter. Orthographic projection centred at 180° longitude, 0° latitude.
Because the moon is tidally locked (meaning the same side always faces Earth), it was not until 1959 that the farside was first imaged by the Soviet Luna 3 spacecraft (hence the Russian names for prominent farside features, such as Mare Moscoviense). And what a surprise – unlike the widespread maria on the nearside, basaltic volcanism was restricted to a relatively few, smaller regions on the farside, and the battered highlands crust dominated. A different world from what we saw from Earth.
Of course, the cause of the farside/nearside asymmetry is an interesting scientific question. Past studies have shown that the crust on the farside is thicker, likely making it more difficult for magmas to erupt on the surface, limiting the amount of farside mare basalts. Why is the farside crust thicker? That is still up for debate, and in fact several presentations at this week's Lunar and Planetary Science Conference attempt to answer this question.
The Clementine mission obtained beautiful mosaics with the sun high in the sky (low phase angles), but did not have the opportunity to observe the farside at sun angles favorable for seeing surface topography. This WAC mosaic provides the most complete look at the morphology of the farside to date and will provide a valuable resource for the scientific community. And it's simply a spectacular sight!
The Lunar Reconnaissance Orbiter Camera (LROC) Wide Angle Camera (WAC) is a push-frame camera that captures seven color bands (321, 360, 415, 566, 604, 643, and 689 nm) with a 57 km swath (105 km swath in monochrome mode) from a 50 km orbit. One of the primary objectives of LROC is to provide a global 100 m/px monochrome (643 nm) base map with incidence angles between 55° and 70° at the equator, lighting that is favorable for morphological interpretations. Each month, the WAC provides nearly complete coverage of the Moon under unique lighting. As an added bonus, the orbit-to-orbit image overlap provides stereo coverage. Reducing all these stereo images into a global topographic map is a big job, which is being led by LROC Team Members from the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR). Several preliminary WAC topographic products have appeared in LROC featured images over the past year (Orientale basin, Sinus Iridum). The WAC topographic dataset will be completed and released later this year.
The global mosaic released today is comprised of over 15,000 WAC images acquired between November 2009 and February 2011. The non-polar images were map-projected onto the GLD100 shape model (WAC derived 100 m/px DTM), while polar images were map-projected on the LOLA shape model. In addition, the LOLA-derived crossover-corrected ephemeris and an improved camera pointing provide accurate positioning (better than 100 m) of each WAC image.
Tarix
noyabr 2009 - fevral 2011
date QS:P,+2050-00-00T00:00:00Z/7,P1319,+2009-11-00T00:00:00Z/10,P1326,+2011-02-00T00:00:00Z/10
Lower-resolution versions: 6000px, 3000px, and 1000px
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA14021.
This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required.See Commons:Licensing.العربية ∙ беларуская (тарашкевіца) ∙ български ∙ català ∙ čeština ∙ dansk ∙ Deutsch ∙ English ∙ español ∙ فارسی ∙ français ∙ galego ∙ magyar ∙ հայերեն ∙ Bahasa Indonesia ∙ italiano ∙ 日本語 ∙ македонски ∙ മലയാളം ∙ Nederlands ∙ polski ∙ português ∙ русский ∙ sicilianu ∙ Türkçe ∙ українська ∙ 简体中文 ∙ 繁體中文 ∙ +/−
Lisenziya
Public domainPublic domainfalsefalse
Annotations
InfoField
This image is annotated: View the annotations at Commons
3870
4350
1530
1350
18000
18000
Mare Moscoviense
2070
11670
810
960
18000
18000
Tsiolkovskiy
2700
7320
1470
1770
18000
18000
Mendeleev
3930
11400
1470
1290
18000
18000
Gagarin
3840
12930
660
660
18000
18000
Pavlov
5640
2190
1110
900
18000
18000
Campbell
6930
1590
1200
840
18000
18000
D'Alembert
11430
8880
1980
1830
18000
18000
Korolev
14760
4170
480
510
18000
18000
Kovalevskaya
12510
10860
1020
870
18000
18000
Galois
8190
14070
1350
1020
18000
18000
Leibnitz
4590
13830
780
660
18000
18000
Jules Verne
11520
13350
1980
1830
18000
18000
Apollo
4230
9540
600
630
18000
18000
Chaplygin
10140
14640
480
420
18000
18000
Maksutov
6540
10200
900
900
18000
18000
Heaviside
12960
5820
810
780
18000
18000
Mach
7260
6360
660
570
18000
18000
Anderson
6060
13020
1800
1680
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18000
Mare Ingenii
11220
5460
420
450
18000
18000
Jackson
8070
15060
930
540
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18000
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fayl, moon, farside, fayl, faylın, tarixçəsi, istifadə, edilən, səhifələr, faylın, qlobal, istifadəsisınaq, göstərişi, ölçüsü, piksel, digər, ölçülər, piksel, piksel, piksel, piksel, piksel, piksel, faylın, orijinalı, 8206, piksel, fayl, həcmi, mime, növü, ima. Fayl Faylin tarixcesi Istifade edilen sehifeler Faylin qlobal istifadesiSinaq gosterisi olcusu 600 600 piksel Diger olculer 240 240 piksel 480 480 piksel 768 768 piksel 1 024 1 024 piksel 2 048 2 048 piksel 18 000 18 000 piksel Faylin orijinali 8206 18 000 18 000 piksel fayl hecmi 85 34 MB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Warning The original file is very high resolution It might not load properly or could cause your browser to freeze when opened at full size To avoid these issues use the ZoomViewer Open in ZoomViewerLower resolution versions 6000px 3000px and 1000px Xulase IzahMoon Farside LRO jpg English Far side of the moon by NASA s Lunar Reconnaissance Orbiter Orthographic projection centred at 180 longitude 0 latitude Because the moon is tidally locked meaning the same side always faces Earth it was not until 1959 that the farside was first imaged by the Soviet Luna 3 spacecraft hence the Russian names for prominent farside features such as Mare Moscoviense And what a surprise unlike the widespread maria on the nearside basaltic volcanism was restricted to a relatively few smaller regions on the farside and the battered highlands crust dominated A different world from what we saw from Earth Of course the cause of the farside nearside asymmetry is an interesting scientific question Past studies have shown that the crust on the farside is thicker likely making it more difficult for magmas to erupt on the surface limiting the amount of farside mare basalts Why is the farside crust thicker That is still up for debate and in fact several presentations at this week s Lunar and Planetary Science Conference attempt to answer this question The Clementine mission obtained beautiful mosaics with the sun high in the sky low phase angles but did not have the opportunity to observe the farside at sun angles favorable for seeing surface topography This WAC mosaic provides the most complete look at the morphology of the farside to date and will provide a valuable resource for the scientific community And it s simply a spectacular sight The Lunar Reconnaissance Orbiter Camera LROC Wide Angle Camera WAC is a push frame camera that captures seven color bands 321 360 415 566 604 643 and 689 nm with a 57 km swath 105 km swath in monochrome mode from a 50 km orbit One of the primary objectives of LROC is to provide a global 100 m px monochrome 643 nm base map with incidence angles between 55 and 70 at the equator lighting that is favorable for morphological interpretations Each month the WAC provides nearly complete coverage of the Moon under unique lighting As an added bonus the orbit to orbit image overlap provides stereo coverage Reducing all these stereo images into a global topographic map is a big job which is being led by LROC Team Members from the German Aerospace Center Deutsches Zentrum fur Luft und Raumfahrt DLR Several preliminary WAC topographic products have appeared in LROC featured images over the past year Orientale basin Sinus Iridum The WAC topographic dataset will be completed and released later this year The global mosaic released today is comprised of over 15 000 WAC images acquired between November 2009 and February 2011 The non polar images were map projected onto the GLD100 shape model WAC derived 100 m px DTM while polar images were map projected on the LOLA shape model In addition the LOLA derived crossover corrected ephemeris and an improved camera pointing provide accurate positioning better than 100 m of each WAC image Tarix noyabr 2009 fevral 2011 date QS P 2050 00 00T00 00 00Z 7 P1319 2009 11 00T00 00 00Z 10 P1326 2011 02 00T00 00 00Z 10Menbe http wms lroc asu edu lroc browse view WAC GL180 see also http photojournal jpl nasa gov catalog PIA14021 Muellif NASA GSFC Arizona State UniversityDiger versiyalar Lower resolution versions 6000px 3000px and 1000px This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration NASA under Photo ID PIA14021 This tag does not indicate the copyright status of the attached work A normal copyright tag is still required See Commons Licensing العربية belaruskaya tarashkevica blgarski catala cestina dansk Deutsch English espanol فارسی francais galego magyar հայերեն Bahasa Indonesia italiano 日本語 makedonski മലയ ള Nederlands polski portugues russkij sicilianu Turkce ukrayinska 简体中文 繁體中文 Lisenziya Public domain Public domain false falseThis file is in the public domain in the United States because it was solely created by NASA NASA copyright policy states that NASA material is not protected by copyright unless noted See Template PD USGov NASA copyright policy page or JPL Image Use Policy Warnings Use of NASA logos insignia and emblems is restricted per U S law 14 CFR 1221 The NASA website hosts a large number of images from the Soviet Russian space agency and other non American space agencies These are not necessarily in the public domain Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI 1 See also PD Hubble and Cc Hubble The SOHO ESA amp NASA joint project implies that all materials created by its probe are copyrighted and require permission for commercial non educational use 2 Images featured on the Astronomy Picture of the Day APOD web site may be copyrighted 3 The National Space Science Data Center NSSDC site has been known to host copyrighted content Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain Unless otherwise noted AnnotationsInfoFieldThis image is annotated View the annotations at Commons3870 4350 1530 1350 18000 18000 Mare Moscoviense 2070 11670 810 960 18000 18000 Tsiolkovskiy 2700 7320 1470 1770 18000 18000 Mendeleev 3930 11400 1470 1290 18000 18000 Gagarin 3840 12930 660 660 18000 18000 Pavlov 5640 2190 1110 900 18000 18000 Campbell 6930 1590 1200 840 18000 18000 D Alembert 11430 8880 1980 1830 18000 18000 Korolev 14760 4170 480 510 18000 18000 Kovalevskaya 12510 10860 1020 870 18000 18000 Galois 8190 14070 1350 1020 18000 18000 Leibnitz 4590 13830 780 660 18000 18000 Jules Verne 11520 13350 1980 1830 18000 18000 Apollo 4230 9540 600 630 18000 18000 Chaplygin 10140 14640 480 420 18000 18000 Maksutov 6540 10200 900 900 18000 18000 Heaviside 12960 5820 810 780 18000 18000 Mach 7260 6360 660 570 18000 18000 Anderson 6060 13020 1800 1680 18000 18000 Mare Ingenii 11220 5460 420 450 18000 18000 Jackson 8070 15060 930 540 18000 18000 Von Karman Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki23 47 19 mart 201418 000 18 000 85 34 MB HuntsterHigh resolution mosaic 04 12 9 aprel 20111 600 1 600 1 44 MB Bubba73 Information Description en 1 Far side of the Moon by NASA 039 s Lunar Recon Orbiter Source http apod nasa gov apod image 1104 farside lro1600 jpg Author NASA LRO Date 2011 Permission other versions Istifade edilen sehifeler Bu sekile olan kecidler Ay Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur af wikipedia org layihesinde istifadesi Maan be wikipedia org layihesinde istifadesi Mora Maskvy bjn wikipedia org layihesinde istifadesi Bulan bs wikipedia org layihesinde istifadesi Mjesec satelit Apollo 11 Lunar Reconnaissance Orbiter Sablon Mjeseceve svemirske letjelice ca wikipedia org layihesinde istifadesi Lluna Topografia de la Lluna cs wikipedia org layihesinde istifadesi Lunar Reconnaissance Orbiter de wikipedia org layihesinde istifadesi Mondruckseite en wikipedia org layihesinde istifadesi Mare Moscoviense Far side of the Moon Hypsometric tints Selenography Lunar Reconnaissance Orbiter Template Multiple image testcases User P T Aufrette sandbox en wikibooks org layihesinde istifadesi Solar System Moon Solar System Print version en wikiversity org layihesinde istifadesi Solar System technical Moon User Marshallsumter Radiation astronomy2 Visuals Draft Keynote lectures Craters by radiation Draft Original research Moon Draft Original research Planets User Marshallsumter Radiation astronomy2 Visuals Quiz User Marshallsumter Rocks Rocky objects Astronomy User Marshallsumter Radiation astronomy Courses Principles Hourly 2 User Marshallsumter Radiation astronomy Courses Principles Midterm quiz User Marshallsumter Radiation astronomy Courses Principles Final quiz Titan Quiz User Marshallsumter Rocks Rocky objects Draft Enceladus Quiz Moon Quiz Stars Sun Heliology Quiz Earth Quiz Stars Reds Quiz Draft Dione Quiz User Marshallsumter Radiation astronomy2 Scattered disks Quiz User Marshallsumter Radiation astronomy1 Kuiper belts Quiz Liquids Liquid objects Moon User Marshallsumter Radiation astronomy Craters es wikipedia org layihesinde istifadesi Colonizacion de la Luna Mare Moscoviense Lunar Reconnaissance Orbiter et wikipedia org layihesinde istifadesi Lunar Reconnaissance Orbiter fa wikipedia org layihesinde istifadesi ماه frr wikipedia org layihesinde istifadesi Benutzer Diskussion קיין ומוויסנדיק פ רעפ ערענצן fr wikipedia org layihesinde istifadesi Face cachee de la Lune glk wikipedia org layihesinde istifadesi مانگ Bu faylin qlobal istifadesine baxin Menbe https az wikipedia org wiki Fayl Moon Farside LRO jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,
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