USAAAO 2020, II кръг — Задача 2
2020 National Astronomy Competition · 10 т.
Instructions (Please Read Carefully)
The top 5 eligible scorers on the NAC will be invited to represent USA at the next IOAA. The next 5 eligible scorers will be invited to join the USA guest team at the next IOAA. In order to qualify for the national team, you must be a high school student with US citizenship or permanent residency.
This exam consists of 3 parts: Short Questions, Medium Questions and Long Questions.
The test must be completed within 2.5 hours (150 minutes).
Please solve each problem on a blank piece of paper and mark the number of the problem at the top of the page. The contestant’s full name in capital letters should appear at the top of each solution page. If the contestant uses scratch papers, those should be labeled with the contestant’s name as well and marked as “scratch paper” at the top of the page. Scratch paper will not be graded. Partial credit will be available given that correct and legible work was displayed in the solution.
This is a written exam. Contestants can only use a scientific calculator for this exam. A table of physical constants will be provided. Discussing the problems with other people is strictly prohibited in any way until the end of the examination period on April 5th. Receiving any external help during the exam is strictly prohibited. This means that the only allowed items are: a scientific calculator, the provided table of constants, a pencil (or pen), an eraser, blank sheets of papers, and the exam. No books or notes are allowed during the exam.
Условие
The star Betelgeuse has recently made news for its abnormal dimming. Although the dimming has now been attributed to dust, we consider in this problem that it was due to radial pulsations. Suppose that Betelgeuse’s mass is 11 solar masses and its radius is 887 solar radii. Furthermore, Betelgeuse is currently rotating such that the tangential velocity of a point on its equator is 5000 m/s (assume Betelgeuse is perfectly spherical). The dimming has increased Betelgeuse’s apparent magnitude by 1.05. You may neglect the contribution of pulsation to the surface velocity.
(a) Assuming contraction and expansion are isothermal, find the (new) radius of the star (in solar radii) needed to account for the dimming.
(b) Assuming no mass loss, find the new angular rotation velocity of the star.
Отговори
- (a) 547 solar radii
- (b) rad/s
Решение
Solution: An increase in apparent magnitude of 1.05 corresponds to a decrease in brightness by a factor of . This is the ratio of the final to the initial luminosity. Applying the Stefan-Boltzmann law, , so the final radius is 547 solar radii.
Apply conservation of angular momentum to find the final angular velocity. The initial angular velocity is rad/s. The initial moment of inertia is kg-m and the final moment of inertia is kg-m. , so rad/s.
Оригинал в Архива: usaaao_second_exam_2020__apr4.pdf · официални решения: usaaao_second_exam_2020__apr4sol.pdf