Toggle menu
310,1 tis.
50
18
525,6 tis.
Hrvatska internetska enciklopedija
Toggle preferences menu
Toggle personal menu
Niste prijavljeni
Your IP address will be publicly visible if you make any edits.

Datoteka:Maxwell Montes, 778-,663,-115.jpg

Izvor: Hrvatska internetska enciklopedija

Vidi sliku u punoj veličini((5.120 × 4.600 piksela, veličina datoteke: 5,28 MB, <a href="/wiki/MIME" title="MIME">MIME</a> tip: image/jpeg))


Logo Wikimedijinog spremnika Ova je datoteka sa stranica Zajedničkog poslužitelja Zaklade Wikimedije i smiju je rabiti drugi projekti. Opis s njezine stranice s opisom datoteke prikazan je ispod.

Sažetak

Opis
English: Venus - Maxwell Montes and Cleopatra Crater

Original Caption Released with Image:

This Magellan full-resolution image shows Maxwell Montes, and is centered at 65 degrees north latitude and 6 degrees east longitude. Maxwell is the highest mountain on Venus, rising almost 11 kilometers (6.8 miles) above mean planetary radius. The western slopes (on the left) are very steep, whereas the eastern slopes descend gradually into Fortuna Tessera. The broad ridges and valleys making up Maxwell and Fortuna suggest that the topography resulted from compression. Most of Maxwell Montes has a very bright radar return; such bright returns are common on Venus at high altitudes. This phenomenon is thought to result from the presence of a radar reflective mineral such as pyrite. Interestingly, the highest area on Maxwell is less bright than the surrounding slopes, suggesting that the phenomenon is limited to a particular elevation range. The pressure, temperature, and chemistry of the atmosphere vary with altitude; the material responsible for the bright return probably is only stable in a particular range of atmospheric conditions and therefore a particular elevation range. The prominent circular feature in eastern Maxwell is Cleopatra. Cleopatra is a double-ring impact basin about 100 kilometers (62 miles) in diameter and 2.5 kilometers (1.5 miles) deep. A steep-walled, winding channel a few kilometers wide breaks through the rough terrain surrounding the crater rim. A large amount of lava originating in Cleopatra flowed through this channel and filled valleys in Fortuna Tessera. Cleopatra is superimposed on the structures of Maxwell Montes and appears to be undeformed, indicating that Cleopatra is relatively young.
Datum
Izvor http://photojournal.jpl.nasa.gov/catalog/PIA00149
Autor NASA/JPL

Licencija

Public domain This 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:
Annotations
InfoField
This image is annotated: View the annotations at Commons

Opisi

Dodajte kratko objašnjenje što predstavlja ova datoteka

Predmeti prikazani u ovoj datoteci

motiv

5. veljače 1996

data size engleski

5 539 123 Bajt

4600 točka

5120 točka

image/jpeg

checksum engleski

7f9ed5e730be8f24c36baaa23a6ebf0dfa6d11db

Povijest datoteke

Kliknite na datum/vrijeme kako biste vidjeli datoteku kakva je tada bila.

Datum/VrijemeMinijaturaDimenzijeSuradnikKomentar
sadašnja00:34, 12. listopad 2013.Minijatura za inačicu od 00:34, 12. listopad 2013.5.120 × 4.600 (5,28 MB)wikimediacommons>Sneeuwschaapbrightness increase: levels [0 255] -> [0 220]

Na ovu sliku vode poveznice sa sljedećih stranica:

Metapodatci