Page:Mathematical collections and translations, in two tomes - Salusbury (1661).djvu/283

understand the same, I have upon this paper transcribed the conclusions that he inferreth from his twelve indagations; the first of which is upon the two observations:

	Of Maurolicus and Hainzelius, from which the Star is collected to have been distant from the centre lesse than 3 semidiameters of the Earth, the difference of Parallaxes being 4 gr. 42 m. 30 sec.	3 semid.
2.	And is calculated on the observations of Hainzelius, with Parall. of 8. m. 30 sec. and its distance from the centre is computed to be more than	25 semid.
3.	And upon the observations of Tycho and Hainzelius, with Parall. of 10 m. and the distance of the centre is collected to be little lesse than	19 semid.
4.	And upon the observations of Tycho and the Landgrave, with Parall. of 14 m. the distance from the centre is made to be about	10 semid.
5.	And upon the observations of Hainzelius and Gemma, with Parall. of 42 m. 30 sec. whereby the distance is gathered to be about	4 semid.
6.	And upon the observations of the Landgrave and Camerarius, with Parall. of 8 m. the distance is concluded to be about	4 semid.
7.	And upon the observations of Tycho and Hagecius, with Parall. of 6 m. and the distance is made	31 semid.
8.	And upon the observations of Hagecius and Vrsinus with Parall. of 43 m. and the stars distance from the superficies of the Earth is rendred	1/2 semid.
9.	And upon the observations of Landgravius and Buschius, with Parall. of 15 m. and the distance from the superficies of the Earth is by supputation	1/48 semid.
10.	And upon the observations of Maurolice and Munocius, with Parall. of 4 m. 30 sec. and the compnted distance from the Earths surface is	1/5 semid.
11.	And upon the observations of Munocius and Gemma, with Parall. of 55 m. and the distance from the centre is rendred	13 semid.

12. And