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Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
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Page 131
Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
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Page 132
Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
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Page 133
Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
×
Page 134
Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
×
Page 135
Suggested Citation:"INDEX." National Research Council. 1972. Astronomy and Astrophysics for the 1970s: Volume 1: Report of the Astronomy Survey Committee. Washington, DC: The National Academies Press. doi: 10.17226/13231.
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Page 136

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Index Absolute lncrtlalaystem, 102 aedYitin of, at cdloiQtionaJ iMthutioftl Ad'¥Ueed cMlizatloM (extraterm-trial), (Tobie), S9 49-;ll • aanllll ott of prod~lo• of PbD's Ad..aced RCUII.Idl Projects A&eftCY, 71 (flawc),S7 AEC,tee Atomic E.ncl:IY Commission ......,cterbtieo or (Table), S9 AVcnll. 4. 71.109 Astrometrk irutrumentJ, recommend~· Aircnft, btUoona, and rocteu., 90-91, lloo ror, 9 121 Asttome-tr)',ll, 102-104 OOIU.,91, 119 com. 104 recommendation for,9 Atomic clocks, I 01 Aircraft telescope, 9 1 Atomic. EnerJ,Y Commlsl~n. 71, 9S Air Force C.mbrld&e Rer.earch At mospheric absorption, 109 Llboratories, 71 Atmo1pberlc seelna, IOS Alf11ow. lOS Atmospheric windows, 44 All wt vek:nath capabllhy, 112, 122 4 Automatic me.asurlna enaJncs, 10<4 AmJno •el<lt, 4 2, 48, 89 Automatic transit drclet, 104 Ammonli, 4 2,47, 102 Automation, te.lesoopo costs, 120 Anpllr diameter nux relation, 79 Auxiliary cl«trOftkl, l22,1ll Anplat rttolutSon, 101, l OS ln the ultraYiokt, 100 BackpoWid rodlotlon, 84 Apt.rtun s:ynthet.:lt, 77 Balloo... 4, 7 1 Arcdbo Radio ()btc:rfttory, 66, 114, "80& ......." 16, 18,19. 27, ) 4 116, 122 "Bladt bolos,- 2S. 29, I II AJJOdadotlofUol>enlties(O< R_,m BronJ.Dklt• ooomolocl'. 24 , 4S Ia AltrODOftiY, Ill Allloctued Un.husitics. lne., 114 Catbon compounds. 41, 42, 43,19, 102 Altcroicb,41 CoJbon dioxide, 4$ Alt.ro..b«J, 104 Cartlon monoxido, 19 Astronomers Carbonaeeolll chondrites, 48 131

132 Index Carbonace-.s, 4S E~ctronOJIIPhic cameras, 81 Catrl"'ton, R. C.. 21 Electrooptlcal deteetoB, 28. 82,83 caruer. A. M.• 58 OOSIS, 120 Centimclcr..wavelenath ante-nnm, 101·102 Elecuoopticaltechno~, 38, 123 <OS IS, I 02, 120 EJemmt abundance~, 82, 94 recommtndation (or. 9 Ekm<-ntary•pndde d)tory,ll Ccnumeter·wawelenath radio tekscopes~ 4 Employment survey, S8 CERN, tee European Ct:nler for Nuclear Eu.ropun Center for Nuclear Re:Karch Research, 118 Cerro Tololo lnler·Americ:an Ob..ervatorr. European southern hemiJphere 113,117,122 telc.scope, 118 Chemical elemenu, 39 Evolution, cosmic, 12-19, 27, 48 abundance of, 24 ExobloiOJY, 49-S2 Clrcumstcllar dust shells, 4), 84 Ex plod ina oores or galaxies, lS-39 CometS, 43, 48,99 E xtratcm:scrlul nutcrial, 48 Computlna requireme nt~~, 94-98 CopernlcuJ, J 3 Feden_l obLigations for bas.lc rtJearch in Corona,raphs, 93 tJtronomy (fiaure), 6 1 Cosmic baCkiJ'OUnd radiation, 17, 18 Feden.l support S4.84 for basJc research in astronomy, 120 Cosmic dull, 41 of pou.nd-basc<t IJUonomy (Tab~). 6S Cosmk: raya, I, 3, 29, 33,39 Firuncbhupport, 61-67 Co.mo~lmodeb,78 Fireball, 16, 17 Co>m0~.12-19,20,84,100,111 For~ehyde,42, 102 Crab nebula, 31, 39, as. &6, 90 Formamidc. •U, 89 pullll, 9S Formic odd, 4 2, I 02 Creation Friednunn, A., model of universe, 13 or new mauer, 38 or the universe, 2 Golactic clullel$, 2S, 27 Cyanoooetylene, 42, 89, 102 Galactic halo, I03 Cr~n ut A, IS Galactic plane, 103 Cr~nus X· I , 90 Galnics, 2, 4, 13, 78, 82, 86, 91,99 disturbed, 4 Oata-handlin& equipment, I 23 explo~lonllln, Il l Deep SpaC» Network , 70 radio, 16 Deportment of Dcfen,., S, 71. 11 2, 11 3 spiral structure, 94 114, 119 stellar content, 80 support ror astronomy, 66 Galileo, 3, 112 Detectors Gamma radiatk)n, 2, 4 ayosenleally eookd, 4 Gamma·raY 1ttronomy, recomme:nda· lnfrutd, 85 lion for. 9 Development or life, 45, 47, 48 GamJN..qy tckscopes, 4 DOD.- Dcpanment of Dcf.rue Camow,G.,I6 Dutt clouds, 4 2, 79 Gaseous nebula, 32 O..·arf s:t.ars, 3 General reblivhy. 38 Dynamical astronomy, 9S, 96 Global Atmospheric Research Oyn1mies, planetary, 111 Pro11am, 97 Globular clusters, 2S, 27, 28, I 03 Eclipse experlmenu, 93 Graphite, 43 Einstein, 13, 19, 24, 2S Graviu.tion, l 5 Elec1ronlc 1echnolol)', 4, 35, 4 1, I 04 Gravitation.ul collapse, 2.S, .S4, 94

/Nice 133 CnY1Urlo.W ...,.,., 33 Cn\'1Urloool nd•rion, 3, 4,19, ~ ..,,,,..., .,,,u"· 2.) 41, « ln:tcrs.tdl:u - ' ' •..,4,1S. . 84. HolooiJble -1 Croud•JC'd utrono.._,. costa, 120 Hoys<adc (rldlo td<-1, 66 HltAO, 1M I up Enerar A.t:tronoiMCal 91. 101 Uhi"'Ctiia of uttn...tokl, 99 lllttrSI. . . moleallo1.~. 71,103 loren~ellu phyolca nd dltmlotrr, J, 9S lo, 4 S Obtcn'atoria l.10toprs..l Hea.y dements.. 27 ll<bum, 17,10.17, 39 Jo•.. n pbneU, 47 llttJChd, w.. u J\lpl1er. 4.S HiiJI.. IIItude Ales, 8S ,.,.w,.. or, 4S, 101 Hiab..[netJY AJironomical Obse:n'alories, 36,87,91 , 106, Ill Kh 1 Pu k National Obttmtorr. 7 1, II). lfia:b,• nellf uuonomk:al PfOStlm, S..S-88 11 7, Ill coolS, 88, II 9 recommtncbtktn (Of. I Ltrae 10lu lele~ I to tc.p.encrJ)' partklca, 4 Lara• spo<o l<lt -. 6 , 91, IOO,IOS, KIP raolutto.., 4 106, 110.113 llip<aol•t- solar ndso lel<soope, 110 ..-rJoosroe. s ..,_.,. •. -.... 89 Luer.I03 ...--... E.. 1),., aadbtloll Laboratory. 71 l.awtnKll ll*lelow, IS L<maii,.,C., I3 H•muon, W., IS Udr: Qboerooarorr. 117 Hyd.roJtn, atoe.t, 4 1,1'9 ure.utntcrrt:tlr..a.. )9.41 llrdr•• ..,.pound•. 41, 43,44 condttkMN suflabk (Of, 4 3 11YW01•• IIIOI<clllca. 41, ~. 91 ..ololioe, II Low-ccmpaature phyQQ, )) IW.. UniYCJthy qdlo ltlcKOpe, 10 IINCOinreoulllm, BI Maa<lloN< doudo, 16 lnfrued aatro..omy, 3, 8).-.8$, 91, 109 lobao<tl< tlelcls, 4 ""'"· 85.110 of whhedwJtft.ll rt('(!Minendatkll\l for,l Ma.anelie IIIII, 79 lftfrared deep a.k)' aurvcy, 91 lobn, 44,99, 102 ln!Wed pllxltt, 80 Masen. inlenteUar. t l, 54 .95.107 lnft~ted radildon, 2. l6 lobJO loso. 99 lmdtutt ofTilcofttlcaJ Attrophylic:l Nu Plaftt.t lnttlun ,., ladk»uuonomie. (P'Oposod), 96, 110 89. 101 lntcpad-"1 U:lcTit.ion CIJMnS, 81 McDonald ~motoey, 117 latdbpnt ~ tltewtlc:N in lllercwr. -lo• of perihelioo of,l4 - .... 1 M ....... c.. ll latafaorncttn. 4 llle~llan,J9 illtrv«< nd optical, I 03 llleteorita. 4), 43 Mldltlooo, I 09 McthaM. 47 l•taplacdc: -ner, II M<tllyt aloohol, 41,19. 101 IAknned&tle-tiud tdttcOpe COils_ llO Wexk:a.a utronoft'ICO. coopenUOft lat<rllltlonalcoor ,......., 118 with, Ill lnterplntt&ty dutt, 41 lolodd IMuldl... 94 lftterpllnet.uy medium, 4.5 W oleculu aslronom,. 9.$, 101 lorcntellat pund dull, 17, 2S, 29, 38, 48 lolo leculca,l, 3, 3~4. 84. 101 Moon, I, 48, 84

134 Index MounI Wilson and Palomar Observa· Nuclear phyoica,33, 94 tories., 117 N\ldear reactioM, 17. 94 lofdky Way .2 Nudei,2 Mllli.meter-wave. antenna, 88-90 Nucleosynthem, 25, 27,28,34,38, 39, COlt$, 90, 119 80, Ill recom~t"10ns for, 8 Number of penoru employed iA Millime1n-wne radio telacopa:, 4 utronomy (flcure), 56 NASA, see Nadom_ Aeronautics and l OAO, see Orbltina Asu-onomica.l Spice Administration Observatories National ACidemy of Sciences, 106 Observatories, unJve.rshy-based, 114 Narional Aeronautics and Space Opticalutronomy, 3, 80-83,113 Admlnlstration, 5, 10, 86, 87. C<lSIO, 8 3, 120 91, 96.100,109,112,114, liS, recommendadont for, 8 119, 123 OptlcollnstrumeniJ, I 06, I 07 budcot for astronomy, 61~3 Optical space astronomy. 98 budaet for utronomy not involvins recomrm.ndation for, 8 sateUit.. (Fiauro), 63 Optical tdescope array, 82 budaeu for 111ronomy sateUile OOSIJ, 120 propomo (FIJUre), 62 Optical teleocopeo support for buic: research in a.stron- lar~,e~t U.S. (Table), 67 omy, Ill u.s.. coUectinc area (FiJUre), 69 National uuonomkal obiCI'VItories., 3, Orbitina Altronomloal ObserYatorioo, 43, 3, 70. 96. 116 44,71,91,99 bud..... 65 O.bitin1 Solar Obsavatories, 23, 71, 92, National Computln1 Cmt<r (propo>ed), 93, 11 0 97,110 recommt-ndadons for, 8 Na·r'onal Jt.adto Astronomy Ob.terYJtory, Orpnic: compounds, 102 77, 89, 114, 122 Orpnlc evolullon, 94 N11ional Scienoe Board, S5 Orpnlc molecules, 4, 48 NarJonal Science foundation, S, 71 , I 06. OSO, see Orbllln& Solar Ob.servatortes 11 3,1 14 , 119 Owens Valley aperture synthesis Basic Rc... rch Cranu, 65-66. 122 Interferometer, 107 budJet for 111ronomy. 65-66, 122 Oxnen compounds, 43 National Uluaviolet SPice Observatory. Oz.one, 99 106 NaVII Retearclt Laboratory, 71,113 Parallax. I 0 3 Neptune, 47 Particle phyJico,21 Neutrinoo,I.4,21,S4 Poalliar plaxiet, 84 Neutron radiation, 22 P cYifll•un. 79 Neutron oun, 19,25, 31, JJ-35, 54, 95, Photocathode, 81 104, Ill Photosnphic unith tubal 104 Newton, Ill Photosraphy, 81 equatioru of motion. 9S Planetary atmospheres, 9 I. 98 theory of pavlution. 9 4 Planetary maua, I 04 NitrOFn. 45, 47 Planetary nebu lao. I0 3 Nitrosen compounds, 43 Planetary orblu, 94. I 04 Novte, 79 Planetary positions., 9 S NSF, see NadonaJ Sdenc:e Foundation Planetary uteiUtes, 48 Nuclear croas sections. 34 Planetary system, 2S Nuclear fusion, 24 Planeu, l.2 , 39,41, 19.84,102

Index 135 "'""' phy~cs. 94, 9$ Silicatn., 41, 4$ ftuto, 79, 101 Site dt'Ydopnw.nt ror r.cllo telescopes. 79 -.lmcuy, I OI Sk>' .....,.•• as -riud 10Pt,31,32 Stiplxr, V. M., 13 Prfl.io4ol:ial evolution., .Cl SmaU Astlonomic:al Sa11UIIes, 71, 91 , 100 Problolocl<ol- 42 Smlthaocuua lutJtvtioD, S Pteplant1ary qm~ft'tl., .U, « Solu acthity, 9), 110 P>torttlet. lll-123 Solu utroMmy COUJ. 9 3, I 20 Proper modon~.o t 03 Sola.r cbtomOJpbe:re, 19,93 Ptotostart, 43 s. Solar oorooa, n . 3s, 19, n , n . 110 Pubors, 2 , 4 , 29, 32-33, 39,54, 77, 86, Solu oosmic n.ys, 21·23, 93 9$, 104 Solu cydo, 19, 9) Solar f•cilitia, re.oommendltion for, 8 Qut ntum chemlat.s, 97 Solar nares, 19, 2 1. 22, 92, 93, 110 Quantum me<haniet:, 19 Solar gnnulldon, 93 Quantum t hooty, 94 Sobr maanetW fie ldJ, 19,93 QuiJin,2,4,16, 18,27, 37,39, S4, 77, Sob.r metlil abuncbnet, 39 79,80.82, 84, 86,9 1,98, 107, 108 Solar nebW., 48 Solar pbyslcs, II 0 lbclar, 4, 101, 102 Sob.r plasma , I I 0 lb4ilt~n belu, 4$, 79 Solar provam, 92-93 R.adk) l!tronomy, l9, 113 Solar lbdlotlon SattWtu, 71 CCMU. 119, 120 $ob.t rnea~. 91 rc.tea~drl tupport at 111\iwnitie:s. 80 Solar ateWtc co•u.. 119 Radio erni.tdoft O( IIIOrml SW$, 79 Solar spcct.Nm, 19 Wloplaxieo, la, 37, n , a6 - bdiocnpll, n bdio-qu.iet compact pluies, 38 Radio radbtion, 4 Solar ··--lara<tl u.s. Solarsys..... . . _.l, 95 Optical (Table), 61 Solar wlod, 21 , 2], $4 Radio IOWce, Qab, ll Solid1ta10 pllysia, )) Jbdio tpcarohel.locn-ph, II 0 Sp.ce amonomy oosts, 119 R.adlo tf:ktcopes, la.raest U.S. (Table), Speoe shuule, l OS 72 Spaoete~soopes,22 , 35 , 42 , 44 , 5 4 ,92, Radio wneknatht,l 100 Rod panu, 2, 2$, 28, 108 (Table), 74 Rod ohlrt, 16, 17, $4, 82, 98 or Spital armt plules, 41 Relativistic: asuophyaics, 95 Star CIUSICII, qet, 80 Rebtlvllfle ooUapee, 4 , 38 Stars, cool, 84 Relltlvlty, 4S, Ill Steli&J evolutk)n,ll , l 4-19, 80, 94, 9S Research lnt«cm or u-uonome:rs (Table), Stellar lotcrlon-, I 7 60 Stellu models, 9$ R.obcruon. H. P., 13 SuatOSQOpc, 7 1 ROClktt PfOIJI""• 5-', 8$ Sttatospbt:rk teltJCOpe, IS, 109 R.R Lyr.. Jtan, 27, 28, 1OJ Sulxlwarfs, 103 Suprs,l9 s A.S• .,. SaWl Astronombl Satdliw: Sul'IUDer W tJtYte. thtotedcal titto- SltW1ll, 4 7, 101 plly1b (p-ood). 97 Soorpl.. X·I, a6 SUA, I , 2, 19-24, 1$,39, $4 , 79, 84, 91, Scyfcrt ..luleo,37, Ja, 86, 108 98 Sikl te emit.don, 41 Sunspots. ll

136 Jndtx Supr.rc:onduc:tor, l4 Univen:ity or Tual, 107-in. telescope, Supc:rJiantt,1S.l7, 9 1 116 Superhtu:roclyne sysums, 108 UnivenHy radio (adlidcs costa, 120 Supnno,.e, 27-29, 31-39,54, 86, Uru\0,47 94 , 111 Supcrpubau, 35 VELA satellites. 71 Support rot utronomy at acadtmk Venus. 4 , « .54, 102 iMtitutions. 66 VLA. set V«J larll Array srnctuouon radUdoa., 32 Verj LarFArroy, 76-80,121,122 costs, 80, 119 Tt:ltiCOpes re.oommend.adon ror. 8 auto matte tenlnaand auldJnc. 82,83 Very-lona-bl;~eline lnte.rf'crometry, JS, refrte-tin.a, 81 101,101,104. 107-109 'Tbeoretlcal aauophyiln, 94-98, Ill , I l l and compul lna. colts, 98, 120 Water, 42, 43,4S reoommcndadon (o r, 8 Water maseu, 108 Than, 47 Wbite dwarrs, l, l.S. 3 L. 103 Tolman, R. C., 13 Whitford report, 3, 4 , 53, SS, 66, 68, Trained manpower, 55-60 70, 120. Il l Wolf·Rayet start, 19 Uhunl, 71, 86, 88, 90 Uhnviokc r~dbtion, 2 X radiation, 2, II, 22 Ultravtolel s~ce uuonomy, 29,84, 91 X 'lay utrooomy, 3, 4 , 14 prQtram co.u., 101 . 119 recommendation for.l rccommcn41 don rOf. 8 X<IY -.,oun4,17, 54, 86, 87 Uni¥aa1 bbd:bodr Miltion, 11 Xfly JOWca,l6 llni'mt<, IIIO<I<k, IS Xflys~. 4.S4 , 19,80 Uni'f'fl'Sity o( Arizona, 90-in. tebcope, 116 Zodiacallil)>t, lOS UalY<nlry or HawaU, sa~•. reletcope, 116

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From the time of the ancient Greeks to the mid-twentieth century, the universe was conceived as of as an unchanging cosmos of fixed stars. The growth of technology, theoretical insight, and deeper understanding of the properties of matter, however, have replaced this view with a steadily expanding universe of galaxies—each galaxy a majestic, solely rotating collection of stars intertwined with dust and gases. Dramatic growth in the tools and techniques of observational astronomy have led to the discovery of explosive events, such as exploding galaxies and quasars, and an almost universal presence of high-energy particles and magnetic fields.

Astronomy and Astrophysics for the 1970s: Volume 1 discusses the future of astronomy and astrophysics and recommends new programs and increased funding of moderate research. It concludes that a balanced and well-planned space-astronomy program with adequate computational facilities is essential. The goal should be one large space telescope. The book also asserts that both large national centers and strong university groups are critical for health, balance and innovation.

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