THE CASE FOR A LIQUID MIRROR IN A LUNAR-BASED TELESCOPE

被引:17
作者
BORRA, EF [1 ]
机构
[1] OBSERV MONT MEGANT,MT MEGANTIC,QUEBEC,CANADA
关键词
INSTRUMENTS;
D O I
10.1086/170053
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I discuss the advantages that a lunar liquid mirror telescope would have over a conventional glass mirror instrument. The very high optical quality obtainable with liquid mirrors and their simplicity make them excellent candidates. The mass of a liquid mirror is an order of magnitude less than the mass of a glass mirror of equal size, resulting in substantially smaller shipping costs. Because liquid mirrors are so simple, a 4-8 m diameter lunar liquid mirror telescope should be feasible at relatively low cost very shortly after the establishment of a lunar base, and even larger mirrors should be feasible at later dates. I discuss some practical considerations. In particular, I consider mercury and gallium (and its eutectic alloys) mirrors, concluding that gallium is preferable to mercury because of its higher reflectivity, lower mass and greater ease of wetting.
引用
收藏
页码:317 / 321
页数:5
相关论文
共 19 条
[1]  
BORRA EF, 1982, J ROY ASTRON SOC CAN, V76, P245
[2]   LIQUID MIRROR TELESCOPES - OBSERVATIONS WITH A 1 METER DIAMETER PROTOTYPE AND SCALING-UP CONSIDERATIONS [J].
BORRA, EF ;
BEAUCHEMIN, M ;
LALANDE, R .
ASTROPHYSICAL JOURNAL, 1985, 297 (02) :846-&
[3]   A DIFFRACTION-LIMITED F/2 1.5 METER DIAMETER LIQUID MIRROR [J].
BORRA, EF ;
CONTENT, R ;
DRINKWATER, MJ ;
SZAPIEL, S .
ASTROPHYSICAL JOURNAL, 1989, 346 (01) :L41-&
[4]   LIQUID MIRROR TELESCOPES AS COSMOLOGICAL TOOLS [J].
BORRA, EF ;
CONTENT, R ;
BOILY, E .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1988, 100 (633) :1399-1404
[5]  
BORRA EF, 1987, PASP, V99, P1129
[6]  
BUNNAGEL R, 1965, Z INSTRUMENTENKD, V73, P214
[7]  
Burke J.D., 1985, LUNAR BASES SPACE AC, P77
[8]   OBSERVATORIES ON THE MOON [J].
BURNS, JO ;
DURIC, N ;
TAYLOR, GJ ;
JOHNSON, SW .
SCIENTIFIC AMERICAN, 1990, 262 (03) :42-49
[9]  
BURNS JO, 1988, ENG CONSTRUCTION OPE, P1083
[10]  
BURNS JO, 1988, NASA CP, V2489