Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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underſtand the ſame, I have upon this paper tranſcribed the
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cluſions that he inferreth from his twelve indagations; the firſt of
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which is upon the two
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The greateſt and
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leaſt elevations of
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the new ſtar differ
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not from each
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ther more than the
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polar allitudes, the
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ſaid ſtar being in
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the Firmnment.
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<
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>Of
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Maurolicus
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and
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Hainzelius,
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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
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gr. 42 m.
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30
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ſec.
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<
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>3
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ſemid.
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<
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>2. And is calculated on the obſervations of
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Hain-zelius,
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with Parall. of 8.
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m. 30 ſec.
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and its di-ſtance from the centre is computed to be more than</
cell
>
<
cell
>25
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"/>
ſemid.
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type
="
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"/>
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>
</
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>
<
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<
cell
>3. And upon the obſervations of
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type
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Tycho
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and
<
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Hain-zelius,
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type
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with Parall. of 10
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m.
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emph.end
type
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and the diſtance of the centre is collected to be little leſſe than</
cell
>
<
cell
>19
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type
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ſemid.
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type
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>
</
row
>
<
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<
cell
>4. And upon the obſervations of
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type
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"/>
Tycho
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emph.end
type
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"/>
and the
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type
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Landgrave,
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emph.end
type
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"/>
with Parall. of 14
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type
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"/>
m.
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emph.end
type
="
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"/>
the diſtance from the centre is made to be about</
cell
>
<
cell
>10
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
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<
cell
>5. And upon the obſervations of
<
emph
type
="
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"/>
Hainzelius
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type
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and
<
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type
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Gemma,
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type
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with Parall. of 42
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emph
type
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"/>
m. 30 ſec.
<
emph.end
type
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italics
"/>
whereby the diſtance is gathered to be about</
cell
>
<
cell
>4
<
emph
type
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"/>
ſemid.
<
emph.end
type
="
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"/>
</
cell
>
</
row
>
<
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<
cell
>6. And upon the obſervations of the
<
emph
type
="
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"/>
Landgrave
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emph.end
type
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"/>
and
<
emph
type
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italics
"/>
Camerarius,
<
emph.end
type
="
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"/>
with Parall. of 8
<
emph
type
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"/>
m.
<
emph.end
type
="
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"/>
the di-ſtance is concluded to be about</
cell
>
<
cell
>4
<
emph
type
="
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"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>7. And upon the obſervations of
<
emph
type
="
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"/>
Tycho
<
emph.end
type
="
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"/>
and
<
emph
type
="
italics
"/>
Hage-cius,
<
emph.end
type
="
italics
"/>
with Parall. of 6
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the diſtance is made</
cell
>
<
cell
>31
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>8. And upon the obſervations of
<
emph
type
="
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"/>
Hagecius
<
emph.end
type
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and
<
emph
type
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italics
"/>
Vr-ſinus
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type
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with Parall. of 43
<
emph
type
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m.
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type
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and the ſtars diſtance from the ſuperficies of the Earth is rendred</
cell
>
<
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>1/2
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type
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"/>
ſemid.
<
emph.end
type
="
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"/>
</
cell
>
</
row
>
<
row
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<
cell
>9. And upon the obſervations of
<
emph
type
="
italics
"/>
Landgravius
<
emph.end
type
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and
<
emph
type
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italics
"/>
Buſchius,
<
emph.end
type
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"/>
with Parall. of 15
<
emph
type
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m.
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emph.end
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and the di-ſtance from the ſuperficies of the Earth is by ſupputation</
cell
>
<
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>1/48
<
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ſemid.
<
emph.end
type
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</
cell
>
</
row
>
<
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<
cell
>10. And upon the obſervations of
<
emph
type
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"/>
Maurolice
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and
<
emph
type
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Munocius,
<
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type
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with Parall. of 4
<
emph
type
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"/>
m. 30 ſec.
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"/>
and the compnted diſtance from the Earths ſurface is</
cell
>
<
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>1/5
<
emph
type
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"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>11. And upon the obſervations of
<
emph
type
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"/>
Munocius
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emph.end
type
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italics
"/>
and
<
emph
type
="
italics
"/>
Gemma,
<
emph.end
type
="
italics
"/>
with Parall. of 55
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the diſtance from the centre is rendred</
cell
>
<
cell
>13
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
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