What powers the Sun? Why does it have spots? How long will it sustain life on Earth? Efforts to answer these questions about the astrophysical object that is of greatest importance to humanity have produced many advances in physics and helped lay the main foundations of astrophysics. The three questions, however, remain to be answered. For example, the best models of the Sun's nuclear power predict a significantly higher neutrino flux than is observed. (See PHYSICS TODAY April, page 19.) We do not know what causes sunspots and other solar activity or even why the Sun emits x rays. Modeling how stars evolve leads to age estimates for some stars that are greater than recent estimates of the age of the universe.

1.
J. N.
Bahcall
,
K.
Lande
,
R. E.
Lanou
,
J. G.
Learned
,
R. G. H.
Robertson
,
L.
Wolfenstein
,
Nature
375
,
29
(
1995
).
2.
Recent comprehensive reviews of helioseismology include:
D. O.
Gough
,
J.
Toomre
,
Annu. Rev. Astron. Astrophys.
29
,
627
(
1991
).
S. V.
Vorontsov
,
Sov. Astron.
36
,
175
(
1992
).
F. Hill et al., in Solar Interior and Atmosphere, Part II, A. N. Cox, W. C. Livingston, M. S. Matthews, eds., Univ. Ariz. Press, Tucson (1991), pp. 329–660.
See also, M. Stix, The Sun, An Introduction, Springer, Berlin (1991).
3.
J. A.
Guzik
,
A. N.
Cox
,
Astrophys. J.
411
,
394
(
1993
).
J. N. Bahcall, M. H. Pinsonneault, Rev. Modern Phys., to appear Oct. 1995.
4.
G.
Grec
,
E.
Fossat
,
Astron. Astrophys.
55
,
411
(
1977
).
J. R.
Brookes
,
G. R.
Isaak
,
H. B. van der
Raay
,
Mon. Not. R. Astron. Soc.
185
,
1
(
1978
).
5.
A.
Cacciani
,
M.
Fofi
,
Sol. Phys.
59
,
179
(
1978
).
S.
Tomczyk
,
K.
Streander
,
G.
Card
,
D.
Elmore
,
H.
Hull
,
A.
Cacciani
,
Solar Phys.
159
,
1
(
1995
).
6.
A. M.
Title
,
H. E.
Ramsey
,
Appl. Opt.
19
,
2046
(
1980
).
J. Harvey and the GONG Instrument Team, in Seismology of the Sun & Sun‐Like Stars, E. J. Rolfe, ed., ESA SP‐286, ESA, Noordwijk, The Netherlands (1988), p. 203.
J. T. Hoeksema, P. H. Scherrer, A. M. Title, T. D. Tarbell, in Seismology of the Sun & Sun‐Like Stars, p. 407.
7.
S. M. Jefferies, M. A. Pomerantz, T. L. Duvall Jr., J. W. Harvey, in Seismology of the Sun & Sun‐Like Stars, p. 279.
8.
P.
Kumar
,
Astrophys. J.
428
,
827
(
1994
).
9.
J.
Christensen‐Dalsgaard
,
T. L.
Duvall
Jr.
,
D. O.
Gough
,
J. W.
Harvey
,
E. J.
Rhodes
Jr.
,
Nature
315
,
378
(
1985
).
10.
F. J.
Rogers
,
C. A.
Iglesias
, in GONG 1992: Seismic Investigation of the Sun and Stars,
T. M.
Brown
, ed.
ASP Conf. Ser.
42
,
155
(
1993
).
11.
J.
Christensen‐Dalsgaard
,
D. O.
Gough
,
M. J.
Thompson
,
Astrophys. J.
378
,
413
(
1991
).
12.
D. O.
Gough
,
A. G.
Kosovichev
,
T.
Toutain
,
Sol. Phys.
157
,
1
(
1995
).
13.
F.‐L.
Deubner
,
R. K.
Ulrich
,
E. J.
Rhodes
Jr.
,
Astron. Astrophys
72
,
177
(
1979
).
14.
T. M.
Brown
et al.,
Astrophys. J.
343
,
526
(
1989
).
15.
Y.
Elsworth
et al.,
Nature
376
,
669
(
1995
).
16.
T. J. Bogden, D. C. Braun, in Proc. 4th SOHO Workshop: Helioseismology, V. Domingo et al., eds., ESA SP‐376, ESA, Noordwijk, The Netherlands, to appear 1995.
17.
The SOHO Mission: Scientific and Technical Aspects of the Instruments, T. D. Guyenne, ed., ESA SP‐1104, ESA, Noordwijk, The Netherlands (1989).
18.
The status of ground‐based networks is described in GONG ‘91: Helio‐ and Astero‐Seismology From the Earth and Space,
R. K.
Ulrich
,
E. J.
Rhodes
Jr.
,
W.
Dappen
, eds.,
ASP Conf. Ser.
76
(
1995
).
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