Brightness of Mars as observed from earth

In summary, the brightness of Mars when in opposition can be explained in both the Ptolemaic and Copernican models of the solar system. In the Ptolemaic model, the deferent and epicycle system show that Mars is closest to Earth at opposition, causing it to appear brighter. In the Copernican model, the retrograde motion of Mars when in opposition also contributes to its increased brightness.
  • #1
lebbo
16
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it is observed that Mars is somewhat brighter when in opposition (ie. sun- Earth - Mars in that order) that at other times. How can this be explained using
a) The Ptolemaic model and
b) The Copernican model of the solar system.
(Assume that Ptolomy's construction describes the actual motion of the planet)

can some one give me some sites and also an explanation
 
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  • #2
lebbo said:
it is observed that Mars is somewhat brighter when in opposition (ie. sun- Earth - Mars in that order) that at other times. How can this be explained using
a) The Ptolemaic model and
b) The Copernican model of the solar system.
(Assume that Ptolomy's construction describes the actual motion of the planet)

These sound an awful lot like homework problems. If so, you need to show some attempts before we can help you.
 
  • #3
ok
In both models Mars is closest to Earth at opposition
and i know that ptolemaic model use epicycles
also that Earth is always in the middle of the sun and Mars which makes it brighter i think i m really confused on this question
 
  • #4
In the Ptolemaic (actually Apollonian/Hipparchan) model the deferent of Mars is just a circle around the Earth as center(did they do deferents in your class?). So the position of the mars's epicycle on its deferent can't be the reason Mars is closer to the Earth at opposition (why? Draw a diagram.). What other degree of freedom does the deferent/epicycle system have? Whatever it might be it's a good place to look for the answer.
 
  • #5
thanks iv got it now, the retrograde causes Mars to get brighter when in oppostion of the sun and earth
 
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FAQ: Brightness of Mars as observed from earth

1. What causes the brightness of Mars as observed from earth to change?

The brightness of Mars as observed from earth changes due to its varying distance from the sun and earth. Mars' orbit is elliptical, so its distance from the sun and earth can range from 128 million to 155 million miles. When Mars is closer to earth and receives more sunlight, it appears brighter.

2. How bright is Mars compared to other planets?

Mars is one of the brightest objects in the night sky, second only to Venus. It is also brighter than Jupiter and Saturn, but not as bright as Mercury. Its brightness can vary greatly depending on its distance from earth and the sun.

3. Is the brightness of Mars always the same?

No, the brightness of Mars is not always the same. As mentioned before, its distance from the sun and earth can vary, causing its brightness to change. Additionally, Mars has seasonal changes due to its axial tilt, which can also affect its brightness.

4. Can we see the brightness of Mars with the naked eye?

Yes, the brightness of Mars can be seen with the naked eye. In fact, it is one of the easiest planets to observe without a telescope. It appears as a bright, red-orange star in the night sky.

5. How can we measure the brightness of Mars as observed from earth?

The brightness of Mars can be measured using a scale called apparent magnitude. The lower the number on the scale, the brighter the object appears. Mars typically has an apparent magnitude between -3 and -2, making it one of the brightest objects in the night sky.

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