USAAAO 2020, I кръг — Задача 8
USAAAO National Astronomy Olympiad First Round 02/10/2020-02/16/2020 · 10 февруари 2020 г. · 1 т.
Указания
This exam contains 8 pages and 30 questions. Each question is worth 1 point, so there are 30 points total. Students MUST take the exam between 02/10/2020-02/16/2020. Proctors must scan students’ responses by 11:59 pm PST on 02/16/2020.
PHYSICAL AND ASTRONOMICAL CONSTANTS
| c | Speed of light in vacuo | |
| e | Elementary charge | |
| Neutron rest mass | ||
| Proton rest mass | ||
| Electron rest mass | ||
| h | Planck’s constant | |
| Hubble’s constant | 70 (km/s)/Mpc | |
| k | Boltzmann’s constant | |
| b | Wien’s constant | |
| G | Gravitational constant | |
| Stefan-Boltzmann constant | ||
| First Radiation Constant | ||
| Second Radiation Constant | ||
| Avogadro constant | ||
| R | Gas constant | |
| Bohr radius | ||
| Bohr magneton | ||
| Solar mass | ||
| Solar radius | ||
| Solar luminosity | ||
| Solar temperature | 5770 K | |
| Earth mass | ||
| Mean Earth radius | ||
| Earth moment of Inertia | ||
| R☾ | Mean Moon radius | |
| M♃ | Mean Jupiter mass | |
| R♃ | Mean Jupiter radius | |
| a♃ | Mean orbital radius of Jupiter | 5.2 AU |
| a☾ | Mean semimajor axis Moon orbit | |
| 1 light year | ||
| 1 AU | Astronomical Unit | |
| 1 pc | Parsec | |
| 1 year | ||
| 1 erg |
ENERGY CONVERSION : 1 joule (J) = electronvolts (eV)
Условие
Kerbyn is a small rocky planet in a circular orbit around a star with a semimajor axis of . Kerbyn has an axial tilt of and a sidereal rotation period of . On the vernal equinox, what is the length of the apparent solar day on Kerbyn? The apparent solar day is defined as the interval between successive crossings of the meridian by the sun.
A.
B.
C.
D.
E.
Отговори
- 06h01m45.1s
Решение
D:
Kerbyn’s orbital velocity is m/s. Let be the difference in length between an apparent solar day and a sidereal day on the vernal equinox. Suppose we start a day with the sun at the meridian; seconds later, the sun returns to the meridian. During this time, Kerbyn moves approximately m, so position of the celestial coordinates of the sun change by rad. Since the movement of the sun on the ecliptic is inclined at to the celestial equator on the vernal equinox, the RA of the sun changes by rad. Kerbyn rotates through rad in s, so , or s.
Оригинал в Архива: 2020_usaaao_first_round.pdf · официални решения: usaaao_first_round_answer_key_2020.pdf