To find the number of light years between two celestial objects, we first find the distance from each object to earth. If we connect the dots between Earth and the two objects, we have a triangle. We to sides lengths of that triangle (the distances between Earth and the objects), and we can measure one angle (the angle at the vertex where Earth is. This is enough information to find the distance between the objects using trigonometry (in this case, the law of cosines).
Finding the distance from Earth to an object can be a bit complex. One commonly used method is to look for a pulsating star. We can figure out the absolute brightness (how bright it is without factoring in distance away) of these stars by how often they pulse. Then we can measure the apparent brightness (how bright it looks to us). We can then use both these values to find the distance to the star. (This also works for some supernovae.)
Another method is to use objects that are considered to be 'standard candles'. These objects do not pulse, but we know the relationship between their absolute brightness, apparent brightness, and distance away.
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The asteroid belt can be found located between Jupiter and Mars. It contains a large number of irregularly shaped celestial bodies.
The apparent brightness of a star is represented by its apparent magnitude, which is a logarithmic scale used to measure the brightness of celestial objects as seen from Earth. The lower the apparent magnitude number, the brighter the star appears in the sky. Each increase of one magnitude corresponds to a brightness factor of 2.5.
A.Mercury and VenusB.Jupiter and SaturnC.Neptune and PlutoD.Mars and Jupiterthe answer is D
A fixed magnet attracts iron objects because the magnet creates a magnetic field that exerts a force on the iron objects. Even though the magnetic field doesn't do any work in the physical sense, it still affects the iron objects by aligning their magnetic domains and creating a force of attraction between the magnet and the objects.
relationship between the number of sides of afigure and the number of vertices