Salusbury, Thomas, Mathematical collections and translations (Tome I), 1667

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            <p type="main">
              <s>
                <pb xlink:href="040/01/371.jpg" pagenum="351"/>
              twice as great as that from the Sun to us) in the ſtar of
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              Saturn
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              is
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              almoſt totally imperceptible, and in
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              Jupiter
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              not very
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              ble, what ſhall we think of the fixed ſtars, which I believe you
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              will not ſcruple to place twice as far off as
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              Saturn
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              ? </s>
              <s>In
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              Mars,
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                <lb/>
              which for that it is nearer to us -------</s>
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            <p type="margin">
              <s>
                <margin.target id="marg667"/>
                <emph type="italics"/>
              In objects far
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              remote, and
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              nous, a ſmall
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              proach or receſſion
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              is imperceptible.
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              </s>
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            <p type="main">
              <s>SIMP. </s>
              <s>Pray Sir, put your ſelf to no farther trouble in this
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              particular, for I already conceive that what hath been ſpoken
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              touching the unaltered apparent magnitude of the fixed ſtars may
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              very well come to paſſe, but what ſhall we ſay of the other
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              ficulty that proceeds from not perceiving any variation in the
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              mutation of aſpect?</s>
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            <p type="main">
              <s>SALV. </s>
              <s>We will ſay that which peradventure may ſatisfie
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              you alſo in this particular. </s>
              <s>And to make ſhort, would you not
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              be ſatisfied if there ſhould be diſcovered in the ſtars face
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              tions that you think ought to be diſcovered, in caſe the annual
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              motion belonged to the Earth?</s>
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            <p type="main">
              <s>SIMP. </s>
              <s>I ſhould ſo doubtleſſe, as to what concerns this
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              ticular.</s>
            </p>
            <p type="main">
              <s>SALV. </s>
              <s>I could wiſh you would ſay that in caſe ſuch a
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                <arrow.to.target n="marg668"/>
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              rence were diſcovered, nothing more would remain behind, that
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              might render the mobility of the Earth queſtionable. </s>
              <s>But
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              though yet that ſhould not ſenſibly appear, yet is not its
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              bility removed, nor its immobility neceſſarily proved, it being
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              poſſible, (as
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              Copernicus
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              affirmeth) that the immenſe diſtance of
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              the Starry Sphere rendereth ſuch very ſmall
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              Phænomena
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                <lb/>
              vable; the which as already hath been ſaid, may poſſibly not
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              have been hitherto ſo much as ſought for, or if ſought for, yet
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              not ſought for in ſuch a way as they ought, to wit, with that
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                <arrow.to.target n="marg669"/>
                <lb/>
              exactneſſe which to ſo minute a punctuality would be neceſſary;
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              which exactneſſe is very difficult to obtain, as well by reaſon of the
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              deficiency of Aſttonomical Inſtruments, ſubject to many
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              tions, as alſo through the fault of thoſe that manage them with leſs
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              diligence then is requiſite. </s>
              <s>A neceſſary argument how little
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              dit is to be given to thoſe obſervations may be deduced from the
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              differences which we find amongſt Aſtronomers in aſſigning the
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              places, I will not ſay, of the new Stars or Comets, but of the fixed
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              ſtars themſelves, even to the altitudes of the very Poles, in
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              which, moſt an end, they are found to differ from one another
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              many minutes. </s>
              <s>And to ſpeak the truth, who can in a Quadrant,
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              or Sextant, that at moſt ſhall have its ſide ^{*} 3. or 4. yards long,
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                <arrow.to.target n="marg670"/>
                <lb/>
              aſcertain himſelf in the incidence of the perpendicular, or in the
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              direction of the ſights, not to erre two or three minutes, which
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              in its circumference ſhall not amount to the breadth of a grain of
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              ^{*}
                <emph type="italics"/>
              Mylet
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              ? </s>
              <s>Beſides that, it is almoſt impoſſible, that the Inſtrument
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                <arrow.to.target n="marg671"/>
                <lb/>
              ſhould be made, and kept with abſolute exactneſſe.
                <emph type="italics"/>
              Ptolomey
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              </s>
            </p>
          </chap>
        </body>
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