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Astronomers have recently observed stars orbiting at very high speeds around an unknown object near

Posted on October 23, 2021 By mobete 3 Comments on Astronomers have recently observed stars orbiting at very high speeds around an unknown object near

Astronomers have recently observed stars orbiting at very high speeds around an unknown object near the center of our galaxy. For stars orbiting at distances of about 1014 m from the object, the orbital velocities are about 106 m/s. Assume the orbits are circular, and estimate the mass of the object, in units of the mass of the sun (MSun = 2x1030 kg). If the object was a tightly packed cluster of normal stars, it should be a very bright source of light. Since no visible light is detected coming from it, it is instead believed to be a supermassive black hole.

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Comments (3) on “Astronomers have recently observed stars orbiting at very high speeds around an unknown object near”

  1. Expert says:
    October 23, 2021 at 11:16 am

    i believe it is b. what was the cause of the big bang

    hope this !

    Reply
  2. Expert says:
    October 23, 2021 at 12:26 pm

    well, you would divide 135 by 33 to get your answer. then that is how many seconds it would take. boardman should fly about 132 m or 4.090909090909091 seconds.

    Reply
  3. jakalenn2018 says:
    October 23, 2021 at 8:06 pm

    The mass of the object is 745000 units of the sun

    Explanation:

    We know that the centripetal force with which the stars orbit the object is represented as

    [tex]F_{c}[/tex] = [tex]\frac{mv^{2} }{r}[/tex]

    and this centripetal force is also proportional to

    [tex]F_{c}[/tex] = [tex]\frac{kMm}{r^{2} }[/tex]

    where

    m is the mass of the stars

    M is the mass of the object

    v is the velocity of the stars = 10^6 m/s

    r is the distance between the stars and the object = 10^14 m

    k is the gravitational constant = 6.67 × 10^-11 m^3 kg^-1 s^-2

    We can equate the two centripetal force equations to give

    [tex]\frac{mv^{2} }{r}[/tex] = [tex]\frac{kMm}{r^{2} }[/tex]

    which reduces to

    [tex]v^{2}[/tex] = [tex]\frac{kM}{r}[/tex]

    and then finally

    M = [tex]\frac{rv^{2} }{k}[/tex]

    substituting values, we have

    M = [tex]\frac{10^{14}*(10^{6})^{2} }{6.67*10^{-11} }[/tex] = 1.49 x 10^36 kg

    If the mass of the sun is 2 x 10^30 kg

    then, the mass of the the object in units of the mass of the sun is

    ==> (1.49 x 10^36)/(2 x 10^30) = 745000 units of sun

    Reply

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