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- Rimae Secchi je dvojice měsíčních brázd dlouhých cca 40 km nacházející se poblíž rovníku jižně od (podle něhož získala své jméno) na okraji Mare Fecunditatis (Moře plodnosti) na přivrácené straně Měsíce. Střední selenografické souřadnice jsou 1,0° S, 44,1° V. Severně se mimo mateřského kráteru nachází také pohoří Montes Secchi, východně v Moři plodnosti leží hřbet . Jižně leží brázda Rima Messier, která protíná měsíční rovník. (cs)
- Rimae Secchi is a system of rilles on the Moon, in northwestern Mare Fecunditatis. They are approximately 40 km long and run along the shore of the mare. Rimae Secchi are named after the nearby crater Secchi which, in turn, is named after an Italian astronomer Angelo Secchi. The name of the rilles was approved by the International Astronomical Union in 1985. In 1974, the name Fossae Secchi was proposed on a map published by the US Defense Mapping Agency, but this name was not adopted (on the Moon, the term Rima is traditionally used instead of Fossa). Before this, during preparation to Apollo 8 and 10 flight, the rilles were informally nicknamed Apollo Rille. The northern end of Rimae Secchi is Y-shaped, and the southern part consists of several separate troughs. Rimae Secchi run along the northwestern rim of a ghost crater (lava-filled crater) of approximately 85 km diameter. The rilles are centered at 1°00′N 44°06′E / 1.0°N 44.1°E. The northern part of Rimae Secchi is surrounded with a dark halo, probably pyroclastic deposits like volcanic ash. Such deposits are common near the edges of lunar maria, including several areas in Mare Fecunditatis. To see this feature, a telescope with an aperture of 20 cm or larger is needed. (en)
- Le Rimae Secchi sono una struttura geologica della superficie della Luna. (it)
- Rimae Secchi – grupa rowów na powierzchni Księżyca o średnicy około 35 km. Znajduje się na północno-zachodnim brzegu Mare Fecunditatis, wzdłuż Montes Secchi, na współrzędnych selenograficznych ☾ 1,0°N 44,0°E/1,000000 44,000000. Nazwa tego systemu kanałów została nadana w 1985 roku przez Międzynarodową Unię Astronomiczną i pochodzi od pobliskiego krateru . (pl)
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- Rimae Secchi je dvojice měsíčních brázd dlouhých cca 40 km nacházející se poblíž rovníku jižně od (podle něhož získala své jméno) na okraji Mare Fecunditatis (Moře plodnosti) na přivrácené straně Měsíce. Střední selenografické souřadnice jsou 1,0° S, 44,1° V. Severně se mimo mateřského kráteru nachází také pohoří Montes Secchi, východně v Moři plodnosti leží hřbet . Jižně leží brázda Rima Messier, která protíná měsíční rovník. (cs)
- Le Rimae Secchi sono una struttura geologica della superficie della Luna. (it)
- Rimae Secchi – grupa rowów na powierzchni Księżyca o średnicy około 35 km. Znajduje się na północno-zachodnim brzegu Mare Fecunditatis, wzdłuż Montes Secchi, na współrzędnych selenograficznych ☾ 1,0°N 44,0°E/1,000000 44,000000. Nazwa tego systemu kanałów została nadana w 1985 roku przez Międzynarodową Unię Astronomiczną i pochodzi od pobliskiego krateru . (pl)
- Rimae Secchi is a system of rilles on the Moon, in northwestern Mare Fecunditatis. They are approximately 40 km long and run along the shore of the mare. Rimae Secchi are named after the nearby crater Secchi which, in turn, is named after an Italian astronomer Angelo Secchi. The name of the rilles was approved by the International Astronomical Union in 1985. In 1974, the name Fossae Secchi was proposed on a map published by the US Defense Mapping Agency, but this name was not adopted (on the Moon, the term Rima is traditionally used instead of Fossa). Before this, during preparation to Apollo 8 and 10 flight, the rilles were informally nicknamed Apollo Rille. (en)
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- Rimae Secchi (cs)
- Rimae Secchi (it)
- Rimae Secchi (en)
- Rimae Secchi (pl)
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