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CANIS MAJOR

 

(Abbreviation: CMa).

 

An original constellation, representing one of Orion’s hunting dogs.  Though dominated by Sirius, it contains several other bright stars, of which one (Adhara) is only just below the first magnitude.  Altogether there are 11 stars brighter then the fourth magnitude:

 

It is interesting to note that three of these stars – Wezea, Aludra, and o² - are extremely luminous.  Compared with them, Sirius is extremely feeble, as it has only 26 times the sun’s luminosity.

 

BRIGHTEST STARS

 

 

STAR

R.A.

DEC

MAG

ABS. MAG.

SPEC

DIST. PC

H

M

S

o

1    z

06

20

18.4

-30

03

48

3.02

-1.7

B3

88    PHURAD

2    b

06

22

41.9

-17

57

22

1.98v

-4.8

B1

220  MIRZAM

      l

06

28

10.1

-32

34

48

4.48

-0.5

B5

17

4    x¹

06

31

51.2

-23

25

06

4.34

-3.9

B1

440

5    x²

06

35

03.3

-22

57

53

4.54

0.6

AO

61

7    n²

06

36

41.0

-19

15

22

3.95

0.0

K1

72

8    n³

06

37

53.3

-18

14

15

4.43

0.0

K1

72

9    a

06

45

08.9

-16

42

58

-1.46

1.4

A1

2.7    SIRIUS

13  k

06

49

50.4

-32

30

31

3.96

-2.5

B2

200

16  o¹

06

54

07.8

-24

11

02

3.86

-6.0

K3

520

14  q

06

54

11.3

-12

02

19

4.07

-0.3

K4

73

19  p

06

55

37.3

-20

08

11

4.68

0.6

gF2

65

20  i

06

56

08.1

-17

03

14

4.38

-3.9

B3

410

21  e

06

58

37.5

-28

58

20

1.50

-4.4

B2

150  ADHARA

22  s

07

01

43.1

-27

56

06

3.46

-5.7

MO

460

24  o²

07

03

01.4

-23

50

00

3.03

-6.8

B3

860

23  g

07

03

45.4

-15

38

00

4.11

-3.4

B8

320  MULIPHEN

25  d

07

08

23.4

-26

23

36

1.86

-8.0

F8

940  WEZEA

27

07

14

15.1

-26

21

09

4.66

-2.9

B3

320

28  w

07

14

48.6

-26

46

22

3.86

-2.3

B3

170

29 UW

07

18

40.3

-24

33

32

4.98v

---

O7.8

----

30  t

07

18

41.4

-24

57

15

4.39

-6.0

O9

1100

31  h

07

24

05.6

-29

18

11

2.44

-7.0

B5

760  ALUDRA

Sirius has a white dwarf companion, mag.8; binary, period 50 years.  Though the companion does not appear faint, it is difficult to see because of the overpowering glare of the primary. The separation ranges between 3” to 11”. 5. It was widest in 1975, spectrum variable. x¹ Is also a spectrum variable, and optically variable over a very small range of less then 0.1 magnitude. 

 

VARIABLES

 

STAR

R.A.

DEC

RANGE

PERIOD,D

SPEC

TYPE

H

M

o

R

07

17.2

-16

18

6.2---6.8

1.14

A9

ALGOL

W

07

05.7

-11

51

6.9---7.5

---

N

IRREGULAR

UW

07

18.6

-24

34

4.7---5.3

4.4

O

b LYRÆ  TYPE

 

CLUSTERS AND NEBULÆ

 

OBJECT

R.A.

DEC

TYPE

NOTES

H

M

o

NGC  2204

06

13.5

-18

35

OPEN CLUSTER

MAG .9. FAIRLY RICH

NGC  2217

06

18.7

-27

14

SPIRAL GALAXY

MAG. 12. TYPE SBa

I         2165

06

19.6

-12

57

PLANETARY

MAG. 12.5 CENTRAL STAR OF MAG. 17

NGC  2243

06

27.6

-31

15

OPEN CLUSTER

MAG. 10. SMALL BUT QUITE RICH

NGC  2287 M.41

06

44.9

-20

41

OPEN CLUSTER

MAG. 4.6 NAKED EYE

NGC  2354

07

12.2

-25

38

OPEN CLUSTER

MAG. 9. FAIRLY RICH

NGC  2360

07

15.4

-15

33

OPEN CLUSTER

MAG. 10 FAIRLY RICH

NGC  2362

07

16.6

-24

52

OPEN CLUSTER

MAG. 10.5. MODERATE

 

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