The Caloris Montes /kəˈlɔːrɪs ˈmɒntiːz/ (Latin for "Heat's Mountains") are a range of mountains on Mercury. They are a system of linear hills and valleys that extend more than 1000 km to the northeast from the mountainous rim of Caloris Basin in the Shakespeare quadrangle (H-3). The range consists of numerous rectilinear massifs 1 to 3 km high and about 10 to 50 km long, mostly elongated radially from the center of the basin and separated by hackly-floored, radial troughs and gouge-like structures.
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| - Caloris Montes (en)
- Caloris Montes (cs)
- Caloris Montes (de)
- Caloris Montes (it)
- Caloris Montes (fr)
- Caloris Montes (sv)
- 卡洛里山脈 (zh)
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| - Caloris Montes (Hory žáru) je nejvyšší pohoří na Merkuru. Je meteoritického původu a nachází se na severovýchodním okraji pánve Caloris Basin (souřadnice 39° 24′ N, 187° 12′ W). Řetězec hor je dlouhý 1000 km a dosahuje výšky přes dva kilometry. Podle pozorování sondy MESSENGER se pohoří skládá z řady paprskovitě uspořádaných hřbetů s příkrými srázy, oddělených příčnými hlubokými propastmi. (cs)
- Die Caloris Montes (aus dem lateinischen Berge der Wärme, Hitze) sind eine Gebirgskette auf dem Merkur. (de)
- Les Caloris Montes (littéralement en français : Montagnes de la chaleur) sont une chaîne de montagnes située sur Mercure dans le . Ce relief a été nommé en référence au point de chaleur le plus élevé de la planète, qui a été mesuré à proximité. (fr)
- I Caloris Montes sono un sistema di rilievi presente sulla superficie di Mercurio, a 31,46° di latitudine nord e 174,15° di longitudine ovest. I monti si trovano in prossimità della regione di Caloris Planitia. I montes sono stati battezzati dall'Unione Astronomica Internazionale con un termine latino che significa letteralmente monti del calore, con riferimento alle temperature estremamente elevate che si raggiungono sulla superficie del pianeta durante il giorno mercuriano. (it)
- Caloris Montes är en bergskedja på Merkurius som omger nedslagskratern Caloris Basin. Topparna i denna bergskedja är omkring 2 kilometer höga. Caloris Montes upptäcktes på fotografier tagna av Mariner 10 år 1974. Caloris Montes befann sig vid terminatorn, linjen som delar dag och natt (dag- och natt hemisfärn), när den upptäcktes av Mariner 10, så bara halva delen bergskedjan var synlig Denna geologiartikel saknar väsentlig information. Du kan hjälpa till genom att lägga till den. (sv)
- 卡洛里山脈(拉丁語:Caloris Montes,直譯為熱的山脈)是位於水星的一個山脈,中心座標位於39°24′N 187°12′W / 39.4°N 187.2°W。 (zh)
- The Caloris Montes /kəˈlɔːrɪs ˈmɒntiːz/ (Latin for "Heat's Mountains") are a range of mountains on Mercury. They are a system of linear hills and valleys that extend more than 1000 km to the northeast from the mountainous rim of Caloris Basin in the Shakespeare quadrangle (H-3). The range consists of numerous rectilinear massifs 1 to 3 km high and about 10 to 50 km long, mostly elongated radially from the center of the basin and separated by hackly-floored, radial troughs and gouge-like structures. (en)
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| - Caloris Montes (Hory žáru) je nejvyšší pohoří na Merkuru. Je meteoritického původu a nachází se na severovýchodním okraji pánve Caloris Basin (souřadnice 39° 24′ N, 187° 12′ W). Řetězec hor je dlouhý 1000 km a dosahuje výšky přes dva kilometry. Podle pozorování sondy MESSENGER se pohoří skládá z řady paprskovitě uspořádaných hřbetů s příkrými srázy, oddělených příčnými hlubokými propastmi. (cs)
- Die Caloris Montes (aus dem lateinischen Berge der Wärme, Hitze) sind eine Gebirgskette auf dem Merkur. (de)
- The Caloris Montes /kəˈlɔːrɪs ˈmɒntiːz/ (Latin for "Heat's Mountains") are a range of mountains on Mercury. They are a system of linear hills and valleys that extend more than 1000 km to the northeast from the mountainous rim of Caloris Basin in the Shakespeare quadrangle (H-3). The range consists of numerous rectilinear massifs 1 to 3 km high and about 10 to 50 km long, mostly elongated radially from the center of the basin and separated by hackly-floored, radial troughs and gouge-like structures. The surfaces of the massifs are hackly. They are best developed along the inner edge of the basin where steep inward-facing scarps are common, grading outward into smaller massifs and blocks. The range marks the crest of most prominent ring structure around Caloris. The type area is the region near 18°, 184.5° (FDS 229). It is thought to be composed of uplifted prebasin bedrock covered by deep-seated late ejecta from Caloris. The inner boundary is approximately the outer limit of crater excavation. The Caloris Montes are similar to the so-called Imbrium sculpture on the Moon. It is generally believed that this type of lineated surface feature resulted from excavations by secondary projectiles when the large basins were formed and, possibly, fracturing and faulting of the planet's crust during the basin formation. The Caloris Montes are only the innermost formation of the Caloris Group of formations produced by the Caloris Basin impact. A gap is present in the Caloris Montes toward the southeast; its origin is unknown, but it is somewhat similar to the gap on the east side of the Imbrium Basin, where the mountain ring cuts the edge of the Serenitatis Basin. On Mercury, however, there is no evidence for the presence of a preexisting basin east of Caloris. (en)
- Les Caloris Montes (littéralement en français : Montagnes de la chaleur) sont une chaîne de montagnes située sur Mercure dans le . Ce relief a été nommé en référence au point de chaleur le plus élevé de la planète, qui a été mesuré à proximité. (fr)
- I Caloris Montes sono un sistema di rilievi presente sulla superficie di Mercurio, a 31,46° di latitudine nord e 174,15° di longitudine ovest. I monti si trovano in prossimità della regione di Caloris Planitia. I montes sono stati battezzati dall'Unione Astronomica Internazionale con un termine latino che significa letteralmente monti del calore, con riferimento alle temperature estremamente elevate che si raggiungono sulla superficie del pianeta durante il giorno mercuriano. (it)
- Caloris Montes är en bergskedja på Merkurius som omger nedslagskratern Caloris Basin. Topparna i denna bergskedja är omkring 2 kilometer höga. Caloris Montes upptäcktes på fotografier tagna av Mariner 10 år 1974. Caloris Montes befann sig vid terminatorn, linjen som delar dag och natt (dag- och natt hemisfärn), när den upptäcktes av Mariner 10, så bara halva delen bergskedjan var synlig Denna geologiartikel saknar väsentlig information. Du kan hjälpa till genom att lägga till den. (sv)
- 卡洛里山脈(拉丁語:Caloris Montes,直譯為熱的山脈)是位於水星的一個山脈,中心座標位於39°24′N 187°12′W / 39.4°N 187.2°W。 (zh)
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