Těreškovová (kráter)
| Kráter Těreškovová | |
|---|---|
| Souřadnice na Měsíci | |
| Selenografická šířka | 28,4° S |
| Selenografická délka | 144,3° V |
| Další údaje | |
| Typ kráteru | |
| Průměr kráteru | 31 km |
| Hloubka | ? |
| Colongitudo | 131° |
| Eponym | Valentina Těreškovová |
Kráter Těreškovová
Kráter Těreškovová, Měsíc
Poloha kráteru Těreškovová (v pravé části mapy rovníkové oblasti Měsíce).
Mare Moscoviense. U levého okraje snímku přibližně uprostřed se nachází dvojice kráterů, Těreškovová je ten větší z nich.
Těreškovová je relativně malý měsíční impaktní kráter nacházející se na severní hemisféře na odvrácené straně Měsíce a tudíž není pozorovatelný přímo ze Země. Má průměr 31 km, pojmenován je podle ruské kosmonautky Valentiny Těreškovové, první ženě ve vesmíru.[1]
Těreškovová leží na západním okraji Mare Moscoviense (Moskevské moře) jihovýchodně od kráteru Feoktistov.
Satelitní krátery
V okolí kráteru se nachází několik dalších kráterů. Ty byly označeny podle zavedených zvyklostí jménem hlavního kráteru a velkým písmenem abecedy.[1]
| Těreškovová | Sel. šířka | Sel. délka | Průměr |
|---|---|---|---|
| U | 28,7° S | 142,8° V | 23 km |
Odkazy
Reference
Literatura
- RÜKL, Antonín. Atlas Měsíce. Praha: Aventinum, 1991. ISBN 80-85277-10-7.
Externí odkazy
Obrázky, zvuky či videa k tématu Těreškovová na Wikimedia Commons - LAC 48, mapa 1:1 000 000 (Lambertova projekce)
Média použitá na této stránce
Moonmap from clementine data.png
cylindrical map projection of the Moon. The Moon's whole surface was mapped by the Clementine spacecraft in 1994, here North is at the top. The dark floor of crater Plato is at the middle top above Mare Imbrium, while the bright floor and rays of crater Tycho is near the middle bottom below Mare Imbrium. Mare Procellarum is at the near left, and Mare Tranquillitatis is just right of centre and Mare Crisium is at the near right. The far left and far right show the contrast of the mostly cratered farside with small isolated mare.
cylindrical map projection of the Moon. The Moon's whole surface was mapped by the Clementine spacecraft in 1994, here North is at the top. The dark floor of crater Plato is at the middle top above Mare Imbrium, while the bright floor and rays of crater Tycho is near the middle bottom below Mare Imbrium. Mare Procellarum is at the near left, and Mare Tranquillitatis is just right of centre and Mare Crisium is at the near right. The far left and far right show the contrast of the mostly cratered farside with small isolated mare.
Moon Map - Equatorial region 45S to 45N - LPC1 - NASA.jpg
NASA lunar chart of equatorial region (latitudes 45S to 45N) 1 : 10.000.000 (LPC-1).
NASA lunar chart of equatorial region (latitudes 45S to 45N) 1 : 10.000.000 (LPC-1).
Mare Moscoviense - Clementine.jpg
en:Mare Moscoviense sits in the Moscoviense basin.Like Mare Marginis, this mare appears to be fairly thin. However, it is clearly centered within a large impact basin. It is also much lower than either the outer basin floor or the farside highlands. The great depth of this mare beneath the nearby highlands probably explains why mare units are so rare on the lunar farside. Very few basins on the farside were deep enough to allow mare volcanism. Thus, while large impact basins are found on both the nearside and farside, large mare are mostly found on the nearside. Mare lavas apparently could reach the surface more often and more easily there. The basin material is of the Nectarian epoch, while the mare material is of the Upper Imbrian epoch. The crater Komarov is seen to the southeast of the mare. You can just make out the crater Titov in the northern regin of the mare.
en:Mare Moscoviense sits in the Moscoviense basin.Like Mare Marginis, this mare appears to be fairly thin. However, it is clearly centered within a large impact basin. It is also much lower than either the outer basin floor or the farside highlands. The great depth of this mare beneath the nearby highlands probably explains why mare units are so rare on the lunar farside. Very few basins on the farside were deep enough to allow mare volcanism. Thus, while large impact basins are found on both the nearside and farside, large mare are mostly found on the nearside. Mare lavas apparently could reach the surface more often and more easily there. The basin material is of the Nectarian epoch, while the mare material is of the Upper Imbrian epoch. The crater Komarov is seen to the southeast of the mare. You can just make out the crater Titov in the northern regin of the mare.