3
3 600 I I nGz 211 i j 1 cos 1 sin 2 4 +371[34 f2041[44 -ZI21[25 1 +381[66 3 4 - 1.27 1 - 6.33 4- 8.70 1 - 1.74 4 4 + 0.30 1 + 1.47 0.90 + 0.18 i- 0.00 +. 0.01 I 5 4 - 0.03 ~ - - 7.07 I + 8.89 - 2.11 4 S cos 1 sin -IT24 1 +9!09 +0.03 I -0.22 - 0.03 - 0.01 0.00 ' +O.OI +0.03 -0.41 I( :::: ! + 1.23 5 5 1 - 0.08 I - 0.32 R em a r q u e I. Nous possCdons maintenant deux tableaux des perturbations de 1221 par Jupiter, Ctablis pour des valeurs assez voisines des ClCments e, i, w, 51 et pour des valeurs trbs diffkrentes de n (1282'1093 et 1329'16154). Pratique- ment, quand on aura trouvC la valeur dCfinitive de n, il suffira d'interpoler les tableaux de perturbations (AN 246.339), et le prCsent tableau, pour avoir la valeur dCfinitive des pertur- bations. D'oh l'utilitk du prCsent tableau. // 0.00 1 +0.04 - 0.06 11 0.00 -0.01 I - 1.87 + 0.48 , + 0.18 Remarque 11. Si la valeur de n Ctait tout h fait exacte, il y aurait lieu de calculer le coefficient de l'argument 3M"-8M; M" Ctant l'anomalie moyenne de la Terre et M l'anomalie de 1221. On a 3nf'-8n=4'17656; la planbte et la Terre revien- draient tous les 5 ans aux m&mes points de leurs orbites si n Ctait exact. La valeur de n n'est pas assez sGre pour faire le calcul rapide par la mCthode de Cauchy (Ann. de Paris 7.165, 296; 8.135-136). 1 5.1 5 31 2.11 +23 59 37.8 i 6.0 1 7 34 50.74 +24 23 17.0 ~ 4.8 13 28 14.32 - 5 53 12.1 I 4.7 23 58 17.12 - 6 24 42.3 3.2 6 39 31.97 +z5 12 16.6 ZB-Sk, 1933 Adt 8. E. de Za ViZZemarqut S. J. ~_____ April 23 )k 25 1 May 3 July 9 Oct. 5 Occultations of stars by the Moon observed during the years 1928-32. By Axel' V. mielsen. +1.8 ~ + 42 3 -1.1 1 - 30 9 +1.3 I -141 I -1.4 1 + 56 29 The observations of occultations published in the present paper were made during the five years 1928-32 with the 135 mm guiding telescope of the reflector of the Aarhus Observatory. The eye-and-ear method was employed and tenths of a second were estimated. The reductions were carried out by Innes' method (AJ 835). Following Prof. Brown's suggestions (AJ 876, 922) the positions of the Moon derived from the Nautical Almanac were corrected as follows: Year Correction 1928 +o.zrzAX 1929-32 + 0.182 AX D D . R D where AX is the variation of the longitude of the Moon per minute. The observations and the results of the reductions are given in Table I. With regard to some of the notations in this Table, see Imzes' paper quoted above. Table 2 gives parti- culars of adopted positions for stars not included in the Nautical Almanac. I am greatly indebted to Dr. V. Guth (Prague) for sending me new positions for two of these stars. The observations had previously ' been forwarded to Prof. Brown, and have been used by him in his yearly dis- cussions of observations of occultations. Table I. Star /Mag., aapp. Gapp. 1 Date 1 U.T. 1 u'-u 1 x-p IPhase 5 B. Cnc 121 Tau 181 B. Gem 2 Vir 30 Psc E Gem E Gem 336 B. Aqr BD+ 8'308 BD+ 11 336 BD+zI 612 x Tau 67 Tau BD+zo 692 3 59 46.89 f20 52 36.4 BD+zo 696 1 8.8 I 4 I 35.77 +21 o 54.8 RD+24 750 8.8 1 5 2 35.25 +24 17 48.2 1 8.0 ' 19 12 24.0 0 7 52.1 o 2 48.0 21 47 44.0 21 23 33.2 I5 50 43.8 19 39 €7.9 19 20 30.8 18 23 58.0 22 20 15.2 20 24 7.6 22 22 18.5 April 12 B 12 21 6 14.1 )) I3 ~ 20 55 14.3 +2.5 I - 20 55 1 D +0.6 1 + 5 6 i D + 836 D +I.O + 29 19 , D +I.O ' + 3 28 D -1.4 + 25 36 D -0.3 I , - 947' D -1.9 I - 6 57 D -0.2 I c 14 41 I D

Occultations of stars by the Moon observed during the years 1928–32

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Page 1: Occultations of stars by the Moon observed during the years 1928–32

3 600 I

I nGz 211

i j 1 cos 1 sin 2 4 +371[34 f2041[44 -ZI21[25 1 +381[66 3 4 - 1.27 1 - 6.33 4- 8.70 1 - 1.74 4 4 + 0.30 1 + 1.47 0.90 + 0.18 i - 0.00 +. 0.01

I

5 4 - 0.03 ~ -

- 7.07 I + 8.89 - 2.11

4

S

cos 1 sin -IT24 1 +9!09 +0.03 I -0.22

- 0.03 - 0.01 0.00 ' +O.OI

+0.03 -0.41

I( :::: ! + 1.23 5 5 1 - 0.08 I - 0.32

R em a r q u e I. Nous possCdons maintenant deux tableaux des perturbations de 1221 par Jupiter, Ctablis pour des valeurs assez voisines des ClCments e , i, w , 51 et pour des valeurs trbs diffkrentes de n (1282'1093 et 1329'16154). Pratique- ment, quand on aura trouvC la valeur dCfinitive de n , il suffira d'interpoler les tableaux de perturbations (AN 246.339), et le prCsent tableau, pour avoir la valeur dCfinitive des pertur- bations. D'oh l'utilitk du prCsent tableau.

/ / 0.00 1 +0.04 - 0.06 1 1 0.00 -0.01

I - 1.87 + 0.48 , + 0.18

Remarque 11. Si la valeur de n Ctait tout h fait exacte, il y aurait lieu de calculer le coefficient de l'argument 3M"-8M; M" Ctant l'anomalie moyenne de la Terre et M l'anomalie de 1221. On a 3nf'-8n=4'17656; la planbte et la Terre revien- draient tous les 5 ans aux m&mes points de leurs orbites si n Ctait exact. La valeur de n n'est pas assez sGre pour faire le calcul rapide par la mCthode de Cauchy (Ann. de Paris 7.165, 296; 8.135-136).

1 5.1 5 31 2.11 +23 59 37.8 i 6.0 1 7 34 50.74 +24 23 17.0 ~ 4.8 13 28 14.32 - 5 53 12.1 I 4.7 23 58 17.12 - 6 24 42.3

3.2 6 39 31.97 +z5 12 16.6

ZB-Sk, 1933 A d t 8. E. de Za ViZZemarqut S. J. ~_____

April 23 )k 25

1 May 3 July 9 Oct. 5

Occultations of stars by the Moon observed during the years 1928-32. By Axel' V. mielsen.

+1.8 ~ + 42 3 -1.1 1 - 30 9 +1.3 I -141 I

-1.4 1 + 56 29

The observations of occultations published in the present paper were made during the five years 1928-32 with the 135 mm guiding telescope of the reflector of the Aarhus Observatory. The eye-and-ear method was employed and tenths of a second were estimated.

The reductions were carried out by Innes' method (AJ 835). Following Prof. Brown's suggestions (AJ 876, 922) the positions of the Moon derived from the Nautical Almanac were corrected as follows:

Year Correction 1928 + o . z r z A X 1929-32 + 0.182 AX

D D . R D

where AX is the variation of the longitude of the Moon per minute.

The observations and the results of the reductions are given in Table I. With regard to some of the notations in this Table, see Imzes' paper quoted above. Table 2 gives parti- culars of adopted positions for stars not included in the Nautical Almanac. I am greatly indebted to Dr. V . Guth (Prague) for sending me new positions for two of these stars.

The observations had previously ' been forwarded to Prof. Brown, and have been used by him in his yearly dis- cussions of observations of occultations.

T a b l e I.

Star /Mag., aapp. Gapp. 1 Date 1 U . T . 1 u'-u 1 x - p IPhase

5 B. Cnc 1 2 1 Tau 181 B. Gem 2 Vir 30 Psc E Gem E Gem

336 B. Aqr BD+ 8'308 B D + 11 336 B D + z I 612 x Tau 67 Tau BD+zo 692 3 59 46.89 f 2 0 5 2 36.4 BD+zo 696 1 8.8 I 4 I 35.77 + 2 1 o 54.8 RD+24 750 8.8 1 5 2 35.25 +24 17 48.2

1 8.0 '

19 12 24.0 0 7 5 2 . 1

o 2 48.0

21 47 44.0 2 1 23 33.2

I5 50 43.8 19 39 €7.9 19 20 30.8 18 23 58.0 22 2 0 15.2

20 24 7.6 22 2 2 18.5

April 12

B 1 2 21 6 14.1 )) I3 ~ 2 0 55 14.3

+2.5 I - 20 55 1 D

+0.6 1 + 5 6 i D + 8 3 6 D

+I.O + 29 19 , D

+ I . O ' + 3 28 D -1.4 + 2 5 36 D

-0.3 I , - 9 4 7 ' D -1.9 I - 6 57 D

-0 .2 I c 14 41 I D

Page 2: Occultations of stars by the Moon observed during the years 1928–32

5 600 I 6

103 Tau ~ S ' P ~ I 5h 3m46:oo +~4~.10'2615

X Cnc 8 16 19.33 +24 I4 55.6 yVir I 1 y Vir I1 J ~

X Vir T Aqr 4.4 j 22 45 52.28 -13 57 52.1

A Tau 4.5 1 4 o 33.53 + Z I 53 38.2

7 14 33.00 +26 4 27.8

1 2 38 4.98 - 1 3 45.3

* 4.5 i 14 15 17.05 -13 2 52.2

c Gem 5.5 i 7 39 50.50 + 2 5 57 1 2 . 7

April 13 i 21h32m22?2 +212

H 15 22 36 8.2 +0.9 - 32 21

)) 2 1 23 29 33.0 i j

16 22 36 30.1 ! -0.8 - 55 16 1 D )) '3 '9 '''3 i[-o.9 - 14 I3 1 D

J ~ I Y I4 2 1 12 12.8

NOV. 20 2 2 50 55.4 -0.7 -174 1 7 ! R

-1.8 ' - 63 8 1 D )) 25 I 23 2.8 + I . Z +154 59 j R

Dec. 15 I 23 4.2 ~ -0.5 + 20 3 i D

134B:Gem : 6.5 1 7 1 2 44.50 +26 49 7.8 BD+26 1564 I 7.3 I 7 23 42.85 +26 2 2 2 1 . 2

32 Tau 3 52 45.13 + Z Z 16 50.7 56 Aqr 6.1 2 2 26 35.33 -14 56 27.8

T Ari 1 5.2 2 45 26.66 + 1 7 10 49.8

~ 5.8 I

415B. Tau 1 6.1 5 56 40.42 + 2 7 34 20.7 47 Gem 1 5.6 7 7 6.25 +26 58 24.0

Febr. 10 , z o 32 2.9 1 +0.8 ~ - 32 I D May

Oct. Nov.

3 I 21 49 44.9 Aug. I 7 1 23 55 59.0

31 ! 16 56 27.2

9 ~ 20 I8 12.7

Dec. 3 ~ 20 46 1.0

D 10 23 13 52.0 R

B D + I I 245 8.0 I 48 54.72 + r z 6 10.6 B D + I I 248 7.2 I 49 47.69 + I Z 20 38.6

12 H1 Ari 1 6.3 ~ I 58 51.78 f 1 3 8 44.7

X Cnc 5.9 8 16 27.50 +24 14 32.6 .37 Leo 5.5 10 13 0.34 +14 4 19.7 BD- 5 3577 8.9 12 45 42.68 - 5 2 7 3.7 BD- 5 3588 8.2 12 48 40.18 - 5 43 5.9 19 Ari : 5.8 2 9 19.18 +14 57 40.9 BD- 0 30 9.4 0 13 20.70 + 0 23 41.5 BD- o 32 8.7 o 13 51.31 + o 12 52.2

5 Ari 4.8 3 10 59.16 +zo 47 43.0 4 Cap 5.3 21 -11 44.93 - 2 0 56 17.6 7 0 Aqr 6.1 22 44 55.33 -10 55 0.6 98 B. Psc 6.3 o 14 18.07 + I 18 39.5 2 7 Ari 6.4 , 2 27 8.49 +17 24 23.7

1931

1 Febr. 2 2 I8 53 30.8 -3.2 + 14 32 D )) 22 19 33 57.9 -1.6 - 13 37 D

' Jan. 26 16 41 15.0

March29 I 10 41.4 -0.4 - 35 2 1 D )) 31 I 3 15.0 f 1 . 4 -

-o.6 -

I0 i April 2 19 16 20.8 +2.0

v 2 20 36 49.7 -1.6 Aug. 6 ! o 39 45.1 I +1.3 ' Sept. 26 2 0 9 14.7 ~ -0.5 1

H 26 20 20 46.7 ~ +0.3 1 + 41 5 2 D o 30 21 4 10.9 1 +I.I ' i 1 4 9 6 R

D )) 15 15 35 37.4 , +O.I - 6-43 L) )) 17 19 4 49.4 I -1.2 - 38 33 D H 20 19 51 10.3 I -1.0 - 17 26 D

Dec. 13 16 38 41.2 1 -2.3 + 7 42

80 Leo

BD+13 302

66 Ari B D + z z 504

354 B. Tau 134B. Gem

B D + 9 142

B D t 1 8 339

B D + z z 505

6.4 1 11 2 2 21.71 + 4 13 58.3 Jan. 20 53 55.5 ~ -1.0 , +167 24 1 R

8.7 1 I 53 2-57 +14 14 29.4 )) 12 19 29 57.2 -1.7 j + 21 52 1 D 7.0 1 I 12 13.01 + 9 25 31.1 Febr. 21 13 11.5 I +0.5 I + 7 33 ~ D

6.1 3 24 28.20 + z z 34 25.4 )) 14 17 27 37.6 1-1.6 8.5 2 39 29.26 +19 8 35.7 )> 13 19 57 26.2 -2.0

8.5 3 29 26.90 +23 9 33.5 o 14 20 33 2.0 +0.8 8.2 3 29 23.96 +23 8 34.5 H 14 20 30 44.8 -0.3 -

6.4 5 16 44.12 + 2 7 53 36.0 R 16 19 53 44.5 -0.9 1 - 9 I I D 6.5 1 7 12 52.72 +26 48 55.7 1 D )) 18 r 8 34 27.6 -0.3 I + 1 7 50

38 B. Aur 6.5 , 5 o 23.21 +27 36 20.5 49 Aur I 5.1 1 6 30 55.90 + 2 8 4 47.2 BD+27 1182 6 34 38.15 +27 52 5.8 i Vir 13 23 9.57 - 1 2 21 33.2 1 7 Tau 3 40 52.46 +23 54 18.1 p Tau 4.3 3 41 11.85 +24 15 3 4 , ~ 20 Tau ~ 4.1 3 41 49-12 +24 9 38.4 17 Tau 3.8 3 40 52.46 +23 54 18.1 q Tau 4.3 3 41 11.85 +24 15 34.2 96 Aqr 27 Tau 3 45 11-00 +23 51 8.7 I. Aqr

1 5.7 23 15 56.21 - 5 29 24.2

1 ::: 1 22 2 49.07 -14 11 50.2

1932

March14 I 22 o 31.8 -3.0 D April 12 1 19 16 45.3 -0.4 I z: :i D

D May 17 20 12 14.8 -4.0 + 9 51 D

D 24 I 55 4.0 -1.1 - 30 21 D D 24 2 6 15.0 -0.1 + 4 o D

2 19 33.5 +I.I +117 40 R

)> 12 21 I 0.5 -0.1 - 36 22 '

Aug. 24 I 37 52.0 -1.3 + 46 15 D

I :: 1 3 3 2.0 +I.8 -166 3 R Oct. 19 14 53.9 - 2 . 2 - 15 1 7 D

1 7 55 52.9 -1.6 I + 46 53 D

I *

)) 1 Dec. I8 37 54.7 -1.2 1 + 26 46 D

Page 3: Occultations of stars by the Moon observed during the years 1928–32

7

b ~ ~ , ~ - f tioas

8 2

7

600 I

T a b l e 2.

Epochs

1894-1910 1884-1904 1880-1924

8

Nov. 2 1

Dez. 13

21

2 0

Star

1 9 ~ 4 6 ~ 1 9 19 19 59 17 37 23 i16 5 23

- B D + 8'308

-Im13?23 -2 22.83 - 2 38.44 - 2 39.93 - 2 24.71 - 2 21.66 - 2 18.50

+I'I 336 + 2 1 612

+5'51?2 -0 18.7 - I 38.2 - 1 45.0 + o 39.2 + o 58.8 + I 20.8

t 2 0 692 + 20" 696 +24 750 +26 1517

7,7 O,IO

7,7 7,7 7,7 7,7

Num- I

oS00 +0!3 I 1 ~ 1 4 ~ 5 0 ? 8 1 Co.01 +0.3 I 13 5.70

0.00+0.3 . I 1 2 50.04 0.00+0.3 I 12 48.53 0.00+0.3 I 13 3.53 o.oo+o.3 I 13 6.54

7,7 0.00+0.3 7,7 1 o.oo+0.3

4 I 1880-1907

I 13 9.70 I 13 13.02

; 11883-1909 1882-1911

2 1889-1911

24 2 7

Proper motion

Bergedorf Mitt. 20

I have derived the p. m. + O S O O ~ , -or04 which was applied. The star possibly belongs to the group of the Hyades. See also Hertzsprzlng BAN I .4

19 25 4 19 22 2 6

Ole Romer Observatory, Aarhus, 1933 Sept.

Star ___.__

BD + 26'1564 + I 1 245 + I I 248 - 5 3577 - 5 3588 - o 30 - 0 32 + 9 142 +13 302 + 18 339 f z z 504 + 2 2 505 + 2 7 1182

Beobachtungen von Plan

- Num- ber of

posi- tions -

5 3 4

8

4 6

3

I

2

I

2

I I

ten

I

Epochs 1 Proper motion 1

1876-1905 I 8 70- I 9 I 6 1903-08 1891

1909-32 1908-32 1902-19 1870 1905-23 1913-23 1913 1912

1902-14

Rergedorf Mitt. 20

Bergedorf Mitt. 20

Schorr, EB.-Lexikon

AN 5507

Bed-Bab. Veroff. 5,5 Bergedorf Mitt. 20

Bergedorf Mitt. 20

Greenwich Cat. 1910

Axel' l7 NieZsen.

a m 243 mm-Merz-Repsold-Refrak tor des As t ronomischen O b s e r v a t o r i u m s i n Kiew. Von S. Tscherny. Vergleichstern * g' i B-N'A. I Nr.1 1932.0-33.0 6 1932.0-33.0 Datum ~ Weltzeit f AU 1 AS iVgl.1 Parall. I a g . app. I

I - ~. -

+ 5 14.19 + 4 50.92 -0 31.20 -0 36.62 -0 41.99 - 0 57.69 - 1 3.11 -1 '7.99 + 4 7.00 + 3 29.09 + 3 18.44 +3 7.95 + 3 5.97 + 3 3.01 + z 58.71 + 2 54.00 + 2 57.02 + 3 22.60 + 3 27.35 + 3 3q.92 + 3 46.94 + 4 14.51 + 4 27.61

+ I 35.7 + 3 57.7 + 4 11.6 1-4 42.7 + 5 15.4 + 6 47,8 + 7 19.2 + 8 45.7 -4 24.5 -0 49.7 +o 9.2 + I 6.6 + I 16.2 + I 33.4 + I 53.2 + z 8.7 + I 43.6

- 1 35.4 -1 53.3 -3 35.9 - 6 25.0 - 7 47.7

- 1 1.0

-0.01 +o.z - 0.01 + 0.2 -0.01 + 0 . 2

-0.01 + 0 . 2

-0.01 f O . 2

- 0.01 + 0.2 -0.01 f O . 2

- 0.01 + 0 .2

-0.01 + 0 . 2

0.00 + 0 . 2

0.00 + 0 . 2

0.00 -I- 0 . 2

0.00 + 0 . 2

+ 0.01 + 0 . 2

0.00 + 0 . 2

+ 0.01 + 0.2 + 0.01 + 0 . 2

+O.OI +o.z f O . 0 1 +o.z + 0.01 + 0.2 + 0.01 + 0 . 2

+O.OI + 0 . 2

+ 0.01 + 0 .2

10 41 28.71 1 0 41 5.44 10 40 25.02

10 40 19.60 10 40 14.22

1 0 39 58.51 10 39 53.09 10 39 38.19 '0 38 5.3.~")

I 0 38 4.09 '0 37 54.45 10 3 7 52.40 10 37 49.49 '0 37 45.74 10 37 40.3'

10 38 8.72

10 38 17.01

10 39 0.50

JO *38 l s . f ) X

1 0 37 43.28

10 38 13.45

1 0 38 32.99

1 0 39 13-58

+ 7'14'20Y4 + 7 4 30.0 + 7 3 10.1

+ 7 3 3.3 + 7 5 26.2 + 7 5 45.8 + 7 6 7.7 + 7 6 29.5

+ O ? I O or0 - 0.03 + 1.6 +O.IO+ 1.7 + 0.04 + 1.4 + 0.07 + 0.6 fo.20 +0.3 +0.27+1.1 +0.29+0.4

+ 9 12 58.8 1-0.21 + 2.c

+ 9 15 20.4 +0.26+ I . ?

+ 9 19 17.9 -0.11-0.3 + 9 19 49.1 i -0.35-t0.r + 9 2 0 21.7 1-0.30 I 0.0

+ 9 2 2 25.7 i - 0 . 2 5 I I>.,{

4-9 21 54.31-0.18 0 . 5

-t-o 2.3 52.3 I q 2s I X . 1

I 0 .I I 5.1.5 - 1 I) $2 5 2 . f '

1 C) A3 50.2 1-0 33 59.9 1 4 34 17.2

+ 9 34 37.2 + 9 34 53.4 + 9 34 28.6 + 9 31 44.7 + 9 31 10.4 + 9 30 5 2 . 5 + 9 29 10.2

+ 9 26 21.3 + 9 24 58.8

0 . 2 0 1 .7 0 . 2 , ; I .I.(] O.?S I 3 . 2

0 . 3 2 t 2.7

0. I 6 + 2.0

- 0.34 + 2. I

+ O . O I + 2 . 1

-0.39 + 1.8 -0.19+2.2 - 0.40 + 2.2

+0.10+3.2 - 0.62 + 3.6

-0.39+4.9 -0.26f6.2 -0.55 + 6.4

0.03 + 4.1

5 5 5 5 5 5 5 5 5 5 5 5 5 5 5