IOAA 2010, China (Problems & Solutions)

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24 Proceedings of 4 th IOAA The 4th IOAA Problems and Solutions z Theoretical Competition z Practical Competition: Data Analysis z Observational Competition z Team Competition z Samples of Problems in Different Languages z Samples of Solutions

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4th International Olympiad on Astronomy and Astrophysics 2010, China (Problems & Solutions)

Transcript of IOAA 2010, China (Problems & Solutions)

  • 24

    Proceedings of 4th IOAA

    The 4th IOAA Problems and Solutions

    z Theoretical Competition z Practical Competition: Data Analysis z Observational Competition z Team Competition z Samples of Problems in Different Languages z Samples of Solutions

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    The 4th IOAA Theoretical Competition

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    Proceedings of 4th IOAA

    Please read these instructions carefully:

    1. Each student will receive problem sheets in English and/or in his/her native language. 2. The time available for answering theoretical problems is 5 hours. You will have 15

    short problems (Theoretical Part 1, Problem 1 to 15), and 2 long problems (Theoretical Part 2, Problem 16 and 17).

    3. Use only the pen that has been provided on your desk. 4. Begin answering each problem on a new page of the notebook. Write down the

    number of the problem at the beginning. 5. Write down your "country name" and your "student code" on the cover of the

    notebook. 6. The final answer in each question or part of it must be accompanied by units and the

    correct number of significant digits (use SI or appropriate units). At most 20% of the marks assigned for that part will be deducted for a correct answer without units and/or with incorrect significant digits.

    7. At the end of the exam put all papers and the notebook inside the envelope and leave everything on your desk.

    8.Please write down logically step by step with intermediate equations/calculations to get the final solution.

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    Short Problem Note: 10 points for each problem

    1) In a binary system, the apparent magnitude of the primary star is 1.0 and that of the secondary star is 2.0. Find the maximum combined magnitude of this system. Solution: Let F1, F2, and F0 be the flux of the first, the second and the binary system, respectively.

    )/lg(5.2)21()/lg(5.2

    21

    21

    FFFFm

    =

    = 5

    So, 4.05.2/121 1010/ ==FF

    )101( 4.01210+=+= FFFF 3

    The magnitude of the binary m is:

    mFFFFm 36.0)/)398.01(lg(5.2)/lg(5.21 1110 =+== 2

    So, mm 64.0= 2) If the escape velocity from a solar mass objects surface exceeds the speed of light, what would be its radius ?

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    Proceedings of 4th IOAA

    Solution:

    cR

    GM

    object

    object >2

    4

    2

    2c

    GMR objectobject < 2

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    3011

    )109979.2(109891.1106726.62