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Since Lacaille's time, the principle stars of Norma have been
redistributed, leaving it with fewer Bayer
stars.
Epsilon Normae is a fixed binary: 4.8, 7.5; PA 335, separation
22.8". Both of these stars also have a spectroscopic companion.
Iota1 Normae is a multiple. AB is a rapid binary with
an orbit of 26.9 years. The Epoch 2000 values are
5.6, 5.8; PA 285, and separation 0.5".
Norma has three variables of (possible) interest:
R Normae is a Mira-type variable: 6.5-13.9, with a period of
507.5 days. The next maximum is scheduled for the last week of February
1997; in 2001 the maximum should occur in the last week of April.
S Normae is a well-known cepheid with a range from 6.1 to 6.8
magnitude, every 9.75 days. It is found in the NGC 6087 cluster (see
below).
Norma has several deep sky objects, including a notable planetary nebula.
NGC 6087 is another cluster, some 3500 light years away, comprised of
forty or so stars, ranging from 7-10 magnitude. The group is two degrees
east of iota1; it includes the cepheid variable S Normae.
Sp 1 is a planetary nebula, rather bright and perfectly circular with a 13 magnitude star in its centre. The planetary nebula is five degrees west-southwest of gamma2 Normae.
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