ephemeride des cometen 1889 … (barnard märz 31) berechnet nach den elementen von herrn prof....

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30 ' M! H. M.T. 8h 9"'24' 9 I 59 9 17 45 8 35 48 7 58 39 8 '5 52 8 3 58 ____. 8 I 29 302 sh I Sm26S94 5 18 25.37 5 16 57.87 5 11 30.65 5 1 I 6.38 5 10 42.61 5 10 20.92 5 10 0.09 Observations of Comet 1889 . . . (Barnard March 31) by E. E. Bm-nard, Astronomer of the Lick Observatory. 9.604 9.658 9.674 9.673 9.657 9.619 9.663 9.664 The following observations are a continuation of those published in .4. N. 2894. The comet was seen on the i1tl1 of April but was so excessively faint from moonlight and haze, that it is On the 15'~ it was excessively faint from moon and haze. thought best not to include the observation in this list. Position angles of the tail. April 3 9h 80:o (3 obs.) r\pril 1'7 9h 75?0 (3 obs.) April 18 9h 78?3 (3 obs.) It could be traced for about KO' to 15'. The tail was very difficult to measure on all the dates. The nucleus is perfectly stellar and about 13 magnitude. -1~46'50 -I 31.96 -3 '5.54 +o 9.21 -0 15.05 -0 38.81 -1 0.50 -1 21.32 I 889 - 6'43'.'3 10.7 - o 4.1 12.7 -1 I 3.9 8.8 + 4 23.3 10.6 -+ 2 30.7 17.5 + o 32.9 16.7 - I 17.9 12.7 - 3 10.5 12.7 April 3 3 5 15 16 '7 18 19 * I 2 3 a 1889.0 1 d 1889.0 -4uthority 5h20m14?30 +16O 7' 19:'s W, 5h519-22 (mean of the two places) 5 19 58.19 +16 o 35.8 Comp. with W, 54519-22 5 XI 22.51 +IS 32 5.5 Comp. with W, 54346 __ - __ 1889 I a I d logr I logd ~ H Juniz9 gh9"' 7' +1z03517 0.3535 0.4991 0.75 Juli I 9 9 12 27.5 3 9 9 12 19.0 0.3543 0.4944 0.76 5 9 7 12 10.2 1 9 3 12 1.0 0,3553 0.4890 0.78 9 8 56 XI 51.5 I1 8 47 II 41.6 0.3565 0.4829 0.80 13 8 35 11 31.3 15 5 8 21 +II 20.6 0.3578 0.4760 0.82 1889 I n 1 d 1 logr 1 logd I H Juli 15 5h8"'2~s +1i020:6 0.3578 0.4760 0.82 '9 7 42 10 57.8 0.3503 0.4684 0.84 23 6 50 , 10 33.0 0.3609 0.4600 0.87 25 6 18 10 19.8 27 5 41 10 6.1 0.3627 0.4508 0.90 '7 8 3 I I 9.4 21 7 18 10 45.7 29 50 9 51.8 31 5 4 '4 + 9 36.9 0.3647 0.4409 0.93 +16' 0' 3079 +16 o 27.4 +IS 56 10.3 +I5 36 23.3 +I5 34 30.7 +I5 32 32.8 +IS 30 42.0 +I5 28 49.4 Mean Places of the Comparison Stars for 1889.0. 0.605 0.646 0.666 0.668 0.649 0.653 0.65 5 O 655 Red. ad 1. app. -0S86 -5!'3 -0.86 -5.3 -0.89 -5.3 -1.07 -5.5 -1.08 -5.5 -1.09 -5.6 -1.09 -5.6 -1.10 -5.6 Ir_ I z I 3 3 3 3 3 h,lf Hamilton I 889 April 20. E. E. Barnard. n = 5"6m325, d = +10'28:1. Berlin 1889 Mai 15. A. Berberich.

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Page 1: Ephemeride des Cometen 1889 … (Barnard März 31) berechnet nach den Elementen von Herrn Prof. Krueger in Astr. Nachr. 2893

3 0 '

M! H. M.T.

8h 9"'24' 9 I 59 9 1 7 45 8 35 48 7 58 39 8 '5 5 2

8 3 58

_ _ _ _ .

8 I 29

302

sh I Sm26S94 5 18 25.37 5 16 57.87 5 1 1 30.65 5 1 I 6.38 5 10 42.61 5 1 0 20.92 5 1 0 0.09

Observations of Comet 1889 . . . (Barnard March 31) by E. E. Bm-nard, A s t r o n o m e r o f t h e L i c k O b s e r v a t o r y .

9.604 9.658 9.674 9.673 9.657 9.619 9.663 9.664

The following observations are a continuation of those published in .4. N. 2894. The comet was seen on the i 1 t l 1 of April but was so excessively faint from moonlight and haze, that it is

On the 1 5 ' ~ it was excessively faint from moon and haze. thought best not to include the observation in this list.

P o s i t i o n a n g l e s o f t h e t a i l . April 3 9h 80:o (3 obs.) r\pril 1'7 9h 75?0 (3 obs.) April 18 9h 78?3 (3 obs.)

I t could be traced for about KO' to 15'. The tail was very difficult to measure on all the dates. The nucleus is perfectly stellar and about 1 3 magnitude.

- 1 ~ 4 6 ' 5 0 - I 31.96 -3 '5.54 +o 9.21 -0 15.05 -0 38.81 - 1 0.50

- 1 21.32

I 889

- 6'43'.'3 10.7 - o 4.1 1 2 . 7 - 1 I 3.9 8.8 + 4 23.3 10.6 -+ 2 30.7 17.5 + o 32.9 16.7 - I 17.9 1 2 . 7

- 3 1 0 . 5 1 2 . 7

April 3 3 5

15 16 ' 7 18 19

* I

2

3

a 1889.0 1 d 1889.0 -4uthority

5h20m14?30 +16O 7 ' 19:'s W, 5h519-22 (mean of the two places) 5 19 58.19 + 1 6 o 35.8 Comp. with W, 54519-22 5 X I 2 2 . 5 1 + I S 32 5.5 Comp. with W, 54346

_ _ - __

1889 I a I d l o g r I logd ~ H

Juniz9 gh9"' 7' +1z03517 0.3535 0.4991 0.75 Juli I 9 9 1 2 2 7 . 5

3 9 9 1 2 19.0 0.3543 0.4944 0.76 5 9 7 1 2 1 0 . 2

1 9 3 1 2 1 .0 0,3553 0.4890 0.78 9 8 56 X I 5 1 . 5

I 1 8 47 I I 41.6 0.3565 0.4829 0.80 13 8 35 11 31.3 15 5 8 2 1 + I I 20.6 0.3578 0.4760 0 . 8 2

1889 I n 1 d 1 l o g r 1 l o g d I H

Juli 1 5 5h8" '2~s +1i020:6 0.3578 0.4760 0.82

' 9 7 42 10 57.8 0.3503 0.4684 0.84

2 3 6 5 0 , 1 0 33.0 0.3609 0.4600 0.87 2 5 6 18 1 0 19.8 2 7 5 4 1 10 6.1 0.3627 0.4508 0.90

' 7 8 3 I I 9.4

21 7 18 1 0 45.7

29 5 0 9 51.8 31 5 4 '4 + 9 36.9 0.3647 0.4409 0.93

+16' 0' 3079 +16 o 27.4 + I S 56 10.3 + I 5 36 23.3 + I 5 34 30.7 + I 5 32 32.8 + I S 30 42.0 + I 5 28 49.4

M e a n P l a c e s o f t h e C o m p a r i s o n S t a r s f o r 1889.0.

0.605 0.646 0.666 0.668 0.649 0.653 0.65 5 O 655

Red. ad 1. app.

-0S86 -5!'3 -0.86 -5.3 -0.89 -5.3 -1.07 - 5 . 5 -1.08 - 5 . 5 -1.09 -5.6 -1.09 -5.6 - 1 . 1 0 -5.6

Ir_ I z I

3 3 3 3 3

h,lf Hamilton I 889 April 20. E. E. Barnard.

n = 5"6m325, d = +10'28:1. Berlin 1889 Mai 1 5 . A. Berberich.