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・ Lada Kaštelan
・ Lada Kozlíková
・ Lada Land VM-01
・ Lada Largus
・ Lada Nadezhda
・ Lada Negrul
・ Lada Nesterenko
・ Lada Niva
・ Lada Priora
・ Lada Revolution
・ Lada Riva
・ Lada Samara
・ Lada Silhouette
・ Lada Sport
・ Lada St. Edmund
Lada Terra
・ Lada Togliatti
・ Lada Vesta
・ Lada VFTS
・ Lada X-1
・ Lada XRAY
・ Lada Žigo
・ Lada, Prešov District
・ Lada-class submarine
・ Ladaai
・ Ladaai Ke Baad
・ Ladabhir
・ Ladadika
・ Ladagada
・ Ladahachandra


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Lada Terra : ウィキペディア英語版
Lada Terra
Lada Terra is a major landmass near the south pole of Venus which is centered at 60°S and 20°E and has a diameter of . It is defined by the International Astronomical Union as one of the three "major landmasses," or terrae, of Venus.〔 The term "landmass" is not analogous to the landmass on Earth, as there are no apparent oceans on Venus. The term here applies to a substantial portion of land that lies above the average planetary radius, and corresponds to highlands. The broad region of Lada Terra contains massive coronae, rift zones, and volcanic plains as well as many other features that scientists use to attempt to piece together the history of this complex planet. The distinctive cross-cutting relationships found in the bedding of Lada Terra have been important in realizing relative ages of the extensional belts and coronae, as well as the complex tesserae features present planet-wide. In 1990 the Venus Radar Mapper revealed the largest outflow channel system on the planet located in the northern region of Lada Terra. Although Lada Terra is generally considered a highland of Venus, the topography is much lower-lying than its northern counterparts Ishtar Terra and Aphrodite Terra. Lada Terra is named after the Slavic goddess of love, Lada.
==Features==

Lada Terra is one of eight distinct regions on the surface of Venus. Ishtar Terra and Aphrodite Terra are the other significant terrae of the planet, located near the northern polar region and the equator, respectively. Lada Terra has a diameter of . and covers most of the south pole region on Venus. The region consists of heavily deformed terrains indicating crustal deformation processes effecting the area in the past.〔 The lowlands are much smoother terrain with very little deformation, which scientists postulate to be relatively young lava flow remnants. The most prominent region is the midlands, where gently sloping topography is disrupted by faults, fractures, and corona, making this area the most complex and studied region in Lada Terra.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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