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- B00962
- Eta Cassiopeiae
- Orange and violet
- The color contrast, best seen with good transparency, is very striking in a
- 350-mm at 145x, but not so in a 75-mm at 90x. This binary is only 6 parsecs
- distant. --Mullaney, McCall
- $
- B02290
- Gamma Arietis (Mesartim)
- Bright white and gray
- Easy in a 75-mm at 45x. --Mullaney, McCall
- $
- B02452
- Alpha Piscium
- Pale green and blue
- A tight pair in small telescopes. Though both stars look white in a 350-mm
- at 145x, other apertures give various color impressions. --Mullaney, McCall
- $
- B02477
- Gamma Andromedae (Almach)
- Orange, emerald?, blue
- Finest colored double, orange and blue, and beautiful in all apertures. The
- comes is also a very close binary, present separation 0.5 second, position
- angle 110 degrees. It is difficult in a 350-mm refractor at 600x, but at that
- magnification it is easy in a 750-mm reflector. --Mullaney, McCall
- $
- B02952
- Iota Cassiopeiae
- Yellowish, blue-white, blue-white
- A fine triple, with blue-white comites 2.3 and 7 seconds from the yellowish
- primary. It is somewhat difficult in telescopes smaller than a 150-mm.
- --Mullaney, McCall
- $
- B03276
- Gamma Ceti (Baten Kaitos)
- Pale yellow and blue
- Attractive, close pair. The color contrast is not obvious in a 75-mm, but
- more definite with a 150-mm or a 350-mm. --Mullaney, McCall
- $
- B03584
- Theta Eridani (Acamar)
- Both white
- Brilliant star. Though it lies half a degree outside a -40 degree
- declination limit, it is one of the brightest doubles in the sky. It is easy
- in a 75-mm at 45x, provided seeing is good at low altitudes. --Mullaney,
- McCall
- $
- B04705
- W (32) Eridani
- Yellow and blue-green
- The color contrast is very vivid in a 350-mm at 145x. --Mullaney, McCall
- $
- B06410
- Beta Orionis (Rigel)
- Blue-white and white
- A blue-white supergiant star with a white, much fainter comes. Just
- resolved in a 75-mm (150x), the pair is beautiful in a 350-mm (145x). The
- comes has been reported by some astronomers as an exceedingly close binary. It
- seems elongated at times in a 750-mm refractor at 550x. --Mullaney, McCall
- $
- B06655
- Eta Orionis
- Both white
- Not easy in a 150-mm, or even a 250-mm, unless the seeing is good, and a
- close pair in a 350-mm at 290x. --Mullaney, McCall
- $
- B06915
- Lambda Orionis (Meissa)
- Pale white and violet
- An easy pair. --Mullaney, McCall
- $
- B06931
- Theta Orionis (Trapezium)
- All pale white
- This beautiful multiple system is imbedded in the Orion Nebula. Six
- components are visible in a 100-mm, and easy in a 250-mm at 160x. Many faint
- red stars are seen in this region with a 750-mm reflector at 600x. Color
- contrasts among the six stars are evident in a 150-mm, and easy in a 350-mm.
- --Mullaney, McCall
- $
- B06937
- Iota Orionis
- White, pale blue, grape red
- A fainter version of Beta Orionis (Rigel). A hint of dim nebulosity around
- Iota is noted with 250-mm and 350-mm apertures. In the same field is the
- double Struve 747 (magnitudes 4.25 and 5.50, separation 36 seconds).
- --Mullaney, McCall
- $
- B07031
- Sigma Orionis
- A multiple star, three components being easily seen in a 75-mm, four with a
- 150-mm at 100x. The bright star has a very difficult, close (0.3-second) comes
- making this a quintuple system. In the same field a little to the west is the
- faint, coarse triple star Struve 761. --Mullaney, McCall
- $
- B07089
- Zeta Orionis (Alnitak)
- Topaz, yellow, light purple, gray
- Has a bright, close comes and a distant, faint one. A difficult group
- requiring good seeing even with a 350-mm. --Mullaney, McCall
- $
- B07557
- Theta Aurigae
- Very unequal, close pair; an interesting sight in a 350-mm, but difficult in
- any telescope much smaller than 250-mm. --Mullaney, McCall
- $
- B08412
- Beta Monocerotis
- All yellow-white
- Finest triple star. The components form a slender triangle of 10 seconds'
- greatest extent. This group is easy in a 150-mm and a beautiful sight in a
- 350-mm. --Mullaney, McCall
- $
- B08804
- 12 Lyncis
- A triple system, nice in a 150-mm. The secondary is 1.7 seconds distant at
- position angle 90 degrees. --Mullaney, McCall
- $
- B08833
- Alpha Canis Majoris (Sirius)
- Brilliant white and yellow
- The brightest star other than the sun dazzles the eye with its brilliance in
- a 750-mm telescope. Under excellent sky conditions, the white-dwarf comes can
- just be seen in a 200-mm at 280x. In a 350-mm at 145x, it is easy when the
- seeing is good, but absolutely invisible in average or poor seeing. In a
- 750-mm reflector with a power of 600, the comes is not much plainer than in a
- 350-mm. --Mullaney, McCall
- $
- B09755
- Delta Geminorum (Wasat)
- Pale white and purple
- Somewhat like Eta Cassiopeiae. --Mullaney, McCall
- $
- B10120
- Alpha Geminorum (Castor)
- Bright white, pale white, orange
- The two very bright stars form a close binary. The faint third star, a
- minute of arc away, is just visible in a 150-mm at 150x. Actually, Castor is a
- sextuple system, since all three visible members are also spectroscopic
- binaries. The Castor group is 14 parsecs from us. --Mullaney, McCall
- $
- B10281
- Kappa Puppis
- Both white
- Resembles Gamma Arietis (Mesartim). It is easy in a 150-mm at 45x.
- $
- B11141
- Zeta Cancri
- Yellow, orange, yellowish (changing)
- An attractive, but difficult, triple. Under average conditions, a 100-mm
- shows only two components. The three are well-resolved in a 250-mm at 320x,
- very easy in a 750-mm refractor at 550x. --Mullaney, McCall
- $
- B12080
- Iota Cancri
- Orange and blue
- Like Beta Cygni (Albireo). It is easily split in a 150-mm at 45x.
- --Mullaney, McCall
- $
- B14177
- Gamma Leonis (Algieba)
- Bright orange and greenish-yellow
- A beautiful pair; a fine sight in a 75-mm. --Mullaney, McCall
- $
- B15537
- Xi Ursae Majoris (Alula Australis)
- Subdued white and grayish-white
- A famous binary system with a period of 60 years. It forms a tight pair.
- --Mullaney, McCall
- $
- B17027
- Delta Corvi (Algorab)
- Pale yellow and purple
- A wide pair. The magnitude contrast is strong in a 350-mm at 145x.
- --Mullaney, McCall
- $
- B17146
- 24 Comae Berenices
- Orange and blue-green
- Thes colors are vivid in larger telescopes. --Mullaney, McCall
- $
- B17270
- Gamma Virginis (Porrima)
- Both white
- One of the best-known binary stars in the sky, with an orbital period cited
- as 172 years. Its components are practically equal in brightness. Well seen
- in a 75-mm. --Mullaney, McCall
- $
- B17556
- Alpha Canum Venaticorum (Cor Caroli)
- Flushed white and pale lilac
- One of the best for small telescopes. Although some observers have seen
- color contrast in this pair, to others both members look blue-white.
- --Mullaney, McCall
- $
- B18133
- Zeta Ursae Majoris (Mizar)
- Brilliant white and pale emerald
- The finest double star in the sky for most moderate instruments. Its
- components are separated by 15 seconds; 4th-magnitude Alcor (g Ursae Majoris)
- is 12 minutes distant. The field is excellent for comparing what the naked eye
- can see with what a telescope reveals. Actually, Mizar-Alcor is a sextuple
- system, since each of the three bright stars is also a spectroscopic binary.
- The group is 27 parsecs from Earth. --Mullaney, McCall
- $
- B18155
- g Ursae Majoris (Alcor)
- The Mizar (Zeta Ursae Majoris)-Alcor field is excellent for comparing what
- the naked eye can see with what a telescope reveals. Actually, Mizar-Alcor is
- a sextuple system, since each of the three bright stars is also a spectroscopic
- binary. The group is 27 parsecs from Earth. --Mullaney, McCall
- $
- B19856
- Epsilon Bootis (Izar)
- Pale orange and bluish-green
- In good seeing, high power on a 75-mm shows the two beautifully-colored
- diffraction discs nearly in contact. --Mullaney, McCall
- $
- B19991
- Xi Bootis
- Yellowish and red
- A visual binary with a period of 150 years. Its colors are easy in a
- 350-mm. Xi Bootis is only 7 parsecs away from us. --Mullaney, McCall
- $
- B20725
- Mu Bootis (Alkalurops)
- A fine triple star, being a wide double whose fainter member is a 2-second
- pair. Best view is with 145x on a 350-mm. --Mullaney, McCall
- $
- B20941
- Delta Serpentis
- Both white
- Offers a fine pair in a 75-mm. --Mullaney, McCall
- $
- B21063
- Zeta Coronae Borealis
- Bright bluish and bright greenish
- This double consists of nearly equal stars. The colors are delicate, but a
- 150-mm telescope or larger makes them definite. --Mullaney, McCall
- $
- B21593
- Xi Scorpii
- Pale white, pale yellow, gray
- A triple, part of an unusual double system. A pair of 5th-magnitude stars
- is 1 second apart, with a 7th-magnitude star 7 seconds off. In the same field
- is the 12-second pair Struve 1999. All five stars are travelling through space
- together. A 75-mm shows only four stars, but high power on a 150-mm splits the
- close pair, thus showing all five. There are hints of color differences in a
- 350-mm (145x). The stars are rather scattered in a 750-mm reflector at 600x.
- --Mullaney, McCall
- $
- B21609
- Beta Scorpii (Graffias)
- Pale white and lilac
- Resembles Zeta Ursae Majoris (Mizar). It is a nice sight in small
- telescopes. In a 350-mm the close and very difficult 10th-magnitude comes of
- the primary could not be seen. Beta Scorpii and Alpha Scorpii (Antares)
- provide an interesting dissimilarity in colors. --Mullaney, McCall
- $
- B21771
- Nu Scorpii
- A colorful double-double, a 2-second pair and a 1-second one about 42
- seconds apart. A 75-mm telescope generally shows only a wide double, but
- sometimes resolves one of the pairs. At high power, but with difficulty, a
- 150-mm shows Nu quadruple. A 350-mm at 290x makes the magnitude and color
- contrasts evident, if seeing is good. --Mullaney, McCall
- $
- B22157
- Alpha Scorpii (Antares)
- Fiery red and emerald green
- A beautiful unequal double star. Because it is only 2.9 seconds from the
- bright primary, the companion is difficult in 150-mm and 200-mm telescopes
- under average conditions, but in good seeing a 250-mm shows it will. On a fine
- night with a 350-mm, this is perhaps the most attractive of all doubles. Even
- when Antares is not resolved, the comes can be recognized as a green tinge to
- one side of the red primary. The pair is a superb sight in a 750-mm refractor
- at 550x. --Mullaney, McCall
- $
- B22351
- 16, 17 Draconis
- Form a triple somewhat like Mu Bootis (Alkalurops), but the brighter
- components are more nearly equal, and the primary has a close comes. Though
- nice in a 150-mm, the system is best seen in a 350-mm at 45x. --Mullaney,
- McCall
- $
- B23277
- Alpha Herculis
- Orange red and bluish-green
- The colors are very intense, even in a 75-mm telescope. The brighter
- comes is a semiregular variable. --Mullaney, McCall
- $
- B23294
- Delta Herculis
- White and purple
- Two unrelated stars at different distances from Earth. --Mullaney, McCall
- $
- B23543
- Rho Herculis
- Attractive in small telescopes. --Mullaney, McCall
- $
- B23797
- Nu Draconis
- Both white
- A pair of perfectly matched stars of equal brightness. This is one of the
- few wide pairs that is attractive in larger telescopes. --Mullaney, McCall
- $
- B24538
- 95 Herculis
- Pale red and pale green
- A pair of bright stars, whose hues are delicate, but persistent in all
- apertures. Both stars look white to many observers. --Mullaney, McCall
- $
- B24641
- 70 Ophiuchi
- Yellow and red
- A famous 88-year binary system. The colors are strong in a 75-mm (150x)
- and 350-mm (145x). --Mullaney, McCall
- $
- B25466
- Alpha Lyrae (Vega)
- Both blue-white
- Vega is a dazzling diamond. To the south lies the faint comes, rather
- difficult in less than a 150-mm. In large refractors having a slight "blue
- excess" in color correction, Vega is nearly pure blue, an amazing sight. Light
- from this star takes 26 years to reach Earth. --Mullaney, McCall
- $
- B25666
- Epsilon Lyrae
- Yellow, ruddy, white, white
- The well-known "Double-Double" rates as the finest multiple star. Both
- close pairs (2.3 and 2.7 seconds) are just resolved by 100x on a 75-mm in
- good seeing. Very easy with a 350-mm, which shows all four stars as white.
- --Mullaney, McCall
- $
- B25991
- Theta Serpentis (Alya)
- Both white
- An easy pair. --Mullaney, McCall
- $
- B26953
- Beta Cygni (Albireo)
- Orange and blue
- A beautiful pair. These colors are much more vivid in a 75-mm than a
- 350-mm, as is often the case with bright stars. --Mullaney, McCall
- $
- B27347
- Delta Cygni
- White and blue-white
- Offers a close binary with components very unequal in brightness. Can be
- split in a 75-mm with good seeing; a splendid sight in a 350-mm at 145x; very
- easy in a 750-mm at 550x. --Mullaney, McCall
- $
- B28965
- Gamma Delphini
- Yellow and pale green
- A pair of bright stars, appears delicately colored in a 350-mm. --Mullaney,
- McCall
- $
- B29509
- 61 Cygni
- Both orange
- A famous long-period binary star. Both components are easily split in a
- 75-mm. At a distance of only 3 parsecs, 61 Cygni is one of the nearest stars.
- --Mullaney, McCall
- $
- B30118
- Beta Cephei (Alfirk)
- White and blue
- Offers an unequal double to users of 75-mm telescopes. --Mullaney, McCall
- $
- B31398
- Zeta Aquarii
- Very white and white
- Fine close binary. In a 100-mm the components appear in contact.
- --Mullaney, McCall
- $
- B31419
- Delta Cephei
- Pale orange and blue
- Easy in a 75-mm at 45x. The primary is a 5.4-day variable star, prototype
- of the Cepheids. --Mullaney, McCall
- @
- Copyright 1983, 1984, 1985, 1986 AstroSoft, Inc. Excerpts from copyrighted
- material are included by permission of Sky Publishing Corporation.