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How can I observe Sgr A* with itelescope.net


Can redshift be measured using fourier?How to find which part of the sky a photo contains?How do I know what I'll be able to see?How do I align my finder scope National Geographic 76/700 EQWhat is it exactly about these flares of infrared light from Sgr A* that “confirms” it is a supermassive black hole?I've seen some stars tonight. What could I possibly have been looking at with these pictures?How did they measure the distance to the center of our galaxy to 0.3% accuracy?Meade ETX-90 with computerized mount slews too far during auto-alignmentHow did they estimate the mass of Sgr A*'s companion G2 without knowing what it was?






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$begingroup$


I've been experimenting with itelescope.net and tried to observe Sgr A*.



I was wondering if there are any suggestions how I can best observe the surrounding stars.










share|improve this question









$endgroup$




















    2












    $begingroup$


    I've been experimenting with itelescope.net and tried to observe Sgr A*.



    I was wondering if there are any suggestions how I can best observe the surrounding stars.










    share|improve this question









    $endgroup$
















      2












      2








      2





      $begingroup$


      I've been experimenting with itelescope.net and tried to observe Sgr A*.



      I was wondering if there are any suggestions how I can best observe the surrounding stars.










      share|improve this question









      $endgroup$




      I've been experimenting with itelescope.net and tried to observe Sgr A*.



      I was wondering if there are any suggestions how I can best observe the surrounding stars.







      telescope photography sgr-a






      share|improve this question













      share|improve this question











      share|improve this question




      share|improve this question










      asked 8 hours ago









      NickpickNickpick

      1204 bronze badges




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          $begingroup$

          I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.



          The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.






          share|improve this answer











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            $begingroup$

            I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.



            The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.






            share|improve this answer











            $endgroup$



















              5













              $begingroup$

              I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.



              The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.






              share|improve this answer











              $endgroup$

















                5














                5










                5







                $begingroup$

                I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.



                The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.






                share|improve this answer











                $endgroup$



                I expect that all the itelescope.net instruments work at visible wavelengths. Therefore you have no chance at all to image the stars around Sgr A*, since it is behind about 25-30 magnitudes of optical extinction.



                The published images you have seen were taken by large telescopes working with adaptive optics in the near-infrared (wavelengths longer than 1.5 $mu$m). At these longer wavelengths the extinction is only 2-3 magnitudes.







                share|improve this answer














                share|improve this answer



                share|improve this answer








                edited 7 hours ago

























                answered 8 hours ago









                Rob JeffriesRob Jeffries

                59.2k4 gold badges123 silver badges194 bronze badges




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