Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ...
About this Item
Title
Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ...
Author
Newton, John, 1622-1678.
Publication
London :: Printed for the author by R. and W. Leybourn, and are to be sold by Thomas Piercepoint ...,
1657.
Rights/Permissions
To the extent possible under law, the Text Creation Partnership has waived all copyright and related or neighboring rights to this keyboarded and encoded edition of the work described above, according to the terms of the CC0 1.0 Public Domain Dedication (http://creativecommons.org/publicdomain/zero/1.0/). This waiver does not extend to any page images or other supplementary files associated with this work, which may be protected by copyright or other license restrictions. Please go to http://www.textcreationpartnership.org/ for more information.
Subject terms
Astronomy -- Early works to 1800.
Planetary theory -- Early works to 1800.
Astronomy -- Mathematics -- Early works to 1800.
Cite this Item
"Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ..." In the digital collection Early English Books Online. https://name.umdl.umich.edu/A52255.0001.001. University of Michigan Library Digital Collections. Accessed May 16, 2024.
Pages
descriptionPage 133
CHAP. 17. Of the Motion of Mercury.
THe forme of calculating the place of this Planet is the same with Venus, the Dimensions of whose orbs we shall give you, as the learned Bullialdus hath computed them, but first we will set down the middle motions thereof to the former time.
The middle motions of Mercury.
An. Christ.
Longit. ☿
Aphel. ☿
Node ☿
1500
352. 53750
248. 73556
039. 85639
80
59. 53472
2. 31611
2. 12417
6
326. 41889
. 17361
. 15917
Iuly
147. 58583
. 01694
. 01528
D 1••
65. 47806
. 00126
. 00117
H 18
3. 06917
P 4564
. 07781
Meane Mot.
234. 70198
251. 24348
42. 15618
Aphel. Snbt.
251. 24348
Rest Anom.
343. 45850
The proportion between the Earths orb, and the orbe of Mercury is as 100. 000 to 38585 Semicentricity in the same parts is, 8105. The parts or greatest inclination 4635. And the angle it selfe 6. 90. In the trian∣gle therefore M E H, of the first Diagram of the former Chapter we have known. 1. The halfe sum of the opposite angles M E H and M H E, 8. 27075 the halfe of 16. 54150 which is the complement of the meane A∣nomaly, 343. 4585 to a circle.
2. The side M E
77170
3. The side M H
16210
Summe
93380 co. ar.
5. 0297462
Differ.
60960
4. 7850449
So tang. halfe sum.
8. 27075
9. 1628126
To tang. halfe differ.
5. 42532
8. 9776037
Difference
2. 84543 Angle M E H
Difference doubled
5. 69086 Angle M B H or the E∣quation to be added to the meane longitude, because the Anomaly is more then a semicircle.
Example.
The meane Longitude of Mercury
234. 70198
Equation adde
5. 69086
Eccentrick place
240. 39284
Node subtract
42. 15618
Argument of Latitude K L
198. 23666
descriptionPage 134
To finde the distance of Mercury from the Sun.
As the sine of MBH
5. 69086 co. ar.
1. 0036592
To the side MH
16210
4. 20978••0
So sine of EMH
16. 54150
9. 4544022
To the side BH
46541
4. 6678444
To finde the Reduction.
As Radius, to cosine of XKL
6. 90
9. 9968431
So tangent of KL
18. 23666
9. 5178453
To tangent of XK
11. 11322
9. 5146884
Reduction
12344
And because the argument of Latitude is more then 180, it must be sub∣tracted from the eccentrick place 240. 39284
And then the eccentrick reduced will be. 240. 26940
To finde the present inclination.
As Radius
To the greatest inclination EB
4635
3. 6660497
So sine of KL.
18. 23666
9. 4954646
To the inclinat. XL
1450
3. 1615143
Which are the parts of inclination agreeing to the common Radius 38585. But the distance of Mercury from the Sun being put for Radius, the inclination will be. 1749
For as Radius DL
38585 co. ar.
5. 41358••5
To Mercury dist. BH or AL
46541
4. 6678444
So is XL
1450
3. 1615143
To XL
1749
3. 2429402
To finde the distance corrected by Curtation.
As AL
46541 co. ar.
5. 3321556
To Radius
10. 0000000
So is XL
1749
3. 2429402
To the sine of LAX
2. 15437
8. 5750958
As Radius
10. 0000000
To AL
46541
4. 6678444
So cosine of LAX
2. 15437
9. 9996929
To AX
46509
4. 6675373
To finde the second inequality of Mercury.
We must have given, 1. The Angle NAS which is to be found by sub∣ductiug the Suns place, from the eccentrick place of Mercury reduced, or this from it, so that less then 6 signes may remain, this remainer is the
descriptionPage 135
Anomaly of the orbe, and the complement thereof is the Angle NAS, or the halfe, is the halfe sum of the opposite angles.
Example.
The eccentrick of Mercury reduced
220. 26940
The Suns true place
154. 07347
Anomaly of the orbe
96. 19593
Complement is NAS
83. 80407
Halfe Anomaly
48. 09796
These given with the sides NA and SA. the Analogies are
As the greater side SA
100895 co. ar.
4. 9961293
Is to Radius
10. 0000000
So is the lesser side NA
46509
4. 6675373
To the tangent of
24. 74799
9. 6636666
Adde
45.
As Radius
To the cotang. of
69. 74799
9. 5669785
So tang. halfe summe
48. 09796
10. 0470559
To tang. halfe difference
22. 35160
9. 6140344
Summe
70. 44956 Angle ANS
Difference
25. 74636 Angle ASN
Because the Suns place was subtracted from the eccentrick of Mercury reduced, therefore the angle of Elongation ASN must be added to the
Suns place.
154. 07347
Elongation ASN adde
25. 74636
True place of Mercury
179. 81983
To finde the distance of Mercury from the Earth.
As the sine of ANS
70. 44956 co. ar.
0. 0257891
To the side AS
100895
5. 0038707
So the sine of NAS
83. 80407
9. 9974556
To the side SN
106442
5. 0271154
To finde the Latitude of Mercury from the Earth.
As the side SX
106442 co. ar.
4. 9728846
Is to Radius
10. 0000000
So is XL
1749
3. 2429402
To the tang. of XSL
0. 94169
8. 2158248
Which is the south Latitude of Mercury.
email
Do you have questions about this content? Need to report a problem?
Please contact us.