Avtory: Bruno Daversin
Perevod: Aleksandr Vol'f
(Po materialam www.lpod.org)
Poyasnenie:
Kopernik odin iz samyh vazhnyh kraterov na Lune.
Vy sprosite kak ya mogu nazvat' chto-libo na Lune "naibolee vazhnym"?
Pozvol'te mne izmenit' pervoe predlozhenie i Vy veroyatno soglasites': Kopernik
samyi vazhnyi
krater na Lune iz-za togo, chemu on nas nauchil. Vot tri uroka, kotorye on nam prepodnes.
Pervyi urok: Pochti stokilometrovyi (v poperechnike on 93 km) Kopernik yavlyaetsya obrazcovym
slozhnym
udarnym kraterom. Dlya kraterov s poperechnikom
bolee 15 kilometrov u Kopernika prisutstvuyut vse
tri tipa obrazovanii: vnutrennie steny s rezkimi obryvami i terrasy, bol'shie otnositel'no
ploskie ploshadki i central'nye piki. Vtoroi urok: Evgenii
Shumeiker ispol'zoval krater
Kopernik v kachestve tipichnogo primera v ego analiticheskoi rabote, posvyashennoi fizike
formirovaniya udarnyh kraterov, ob'yasnyayushei proishozhdenie obrazovanii, perechislennyh
vyshe,
a takzhe vtorichnye kratery i luchi. Tretii urok: Kopernik
okazalsya bolee slozhen, chem my schitali.
Ya eto obnaruzhil, kogda sravnival ego s drugimi bolee pozdnimi kraterami so slozhnoi
strukturoi.
Tak Kopernik okazalsya slishkom melkii (poryadka 700 metrov), a central'nye piki dovol'no
nizkimi (poryadka odnogo kilometra). Takim obrazom Kopernik
zapolnen v predelah ot 0.7 do 1.0 km neizvestnym materialom.
Vryad li eto mozhno ob'yasnit' oplavleniem (takoi sloi dolzhen byt' poryadka chetverti
kilometra), vprochem
takzhe kak i drugoi variant - potokami lavy. Poslednii variant voobshe ne lyubyat, potomu
chto iz etogo
sleduet, chto Luna byla sravnitel'no nedavno goryachei - poryadka 1 milliarda let nazad.
Odnako dlya togo, chtoby voshishat'sya etim prevoshodnym snimkom, sdelannym Bruno Daversinom
s ispol'zovaniem 24-h dyuimovogo teleskopa observatorii Lyudiver (Ludiver),
vovse ne nuzhno znat'
iz chego sostoit material na dne kratera - eto mozhet byt' lava, ili mozhet on obrazovalsya
v
rezul'tate oplavleniya v rezul'tate udarnogo vozdeistviya, a mozhet eto imenno sluchainye
otkloneniya
ot srednih znachenii dlya analogichnyh kraterov.
(Po materialam www.lpod.org)
Tehnicheskie detali:
Image obtained 2003 october 18th, 04h33 UT with Ludiver Observatory (Normandy,
France) 600 mm (24") F/D=16
cassegrain telescope + infrared filter + TouCam Pro in B&W mode.
Seeing: 7/10 Pickering. Processed with IRIS
freeware: 400 frames registred, addition, vancittert filter applied.
South is up.
Dopolnitel'nye ssylki:
Ludiver Observatory
and Planetarium Moon Atlas
Clementine
Multispectral view and floor evidence
Vidy Lunar Orbiter
V
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Moon - Luna - Lunar Photo of the Day - LPOD
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