USAAAO 2025, I кръг — Задача 9
USAAAO 2025 - First Round · 8 февруари 2025 г.
Внимание: Бележка към темата
All 30 separately numbered original first-round multiple-choice questions and their matching official explanations/answer letters are retained. The printed explanations for Questions 2 and 3 stop before a promised formula; Question 26 refers to a following triangle absent from its native solution page. No missing expression or diagram is reconstructed. Native scientific discrepancies and ambiguous formula notation remain literal and are explicitly attributed in local source notes. A separate two-page common USAAAO archive constants/reference table is included with its own source identity; it is undated in the catalogue, and its use as the exact 2025 attachment is not established. No separate dated instructions, answer sheet or constants companion is present in the 2025 archive folder. No point total or time limit is printed in these two exam booklets.
Original first-round date and writers
USAAAO 2025 - First Round
February 8th, 2025
Writers: Abhay Bestrapalli, Sidhant Chaliha, Ferdinand, Ved Gund, Hagan Hensley, Yehong Jiang, Alexander Li, Joe McCarty, Lucas Carrit Delgado Pinheiro, Sahil Pontula.
Common archive reference — Table of Physical Constants
This separate common USAAAO archive reference is undated in the catalogue. Its use as the exact 2025 exam attachment is not established.
| Quantity | Symbol | Value |
|---|---|---|
| Electron rest mass | ||
| Proton rest mass | ||
| Electronic charge | ||
| Speed of light in free space | ||
| Permeability of free space | ||
| Permittivity of free space | ||
| Planck’s constant | ||
| Reduced Planck’s constant | ||
| Boltzmann’s constant | ||
| Gas constant | ||
| Molar gas constant | ||
| Avogadro’s number | ||
| Standard molar volume | ||
| Unified atomic mass unit ( scale) | ||
| Mass of hydrogen atom | ||
| Bohr magneton | or | |
| Nuclear magneton | or | |
| Proton magnetic moment | ||
| Neutron magnetic moment | ||
| Bohr radius | ||
| Fine structure constant | ||
| Compton wavelength of electron | ||
| Rydberg’s constant | ||
| Stefan-Boltzmann constant | ||
| Radiation density constant | ||
| Gravitational constant |
Rest masses of some leptons and hadrons in :
0.5110, 105.66, 1777, 134.98, 139.57, 493.7, 497.7, 547, 1865, 1869, p 938.3, n 939.6, 1115.7, 1189, 1193, 1197, 1315, 1321, 1672, , .
| Quark | Charge | Mass () | |||||
|---|---|---|---|---|---|---|---|
| u | 0 | 0 | 0 | 0 | |||
| d | 0 | 0 | 0 | 0 | |||
| c | 0 | 0 | +1 | 0 | 0 | ||
| s | 0 | -1 | 0 | 0 | 0 | ||
| t | 0 | 0 | 0 | 0 | +1 | 174.3 | |
| b | 0 | 0 | 0 | -1 | 0 | 4.2 |
Common archive reference — Astrophysical Data and identities
Astrophysical Data
| Quantity | Symbol | Value |
|---|---|---|
| 1 astronomical unit | AU | |
| 1 parsec | pc | |
| Luminosity of Sun | ||
| Mass of Sun | ||
| Radius of Sun | ||
| Mass of Earth | ||
| Radius of Earth |
Other data and conversion factors
| Quantity | Symbol | Value |
|---|---|---|
| 1 ångstrom | Å | |
| 1 fermi | fm | |
| 1 barn | b | |
| 1 pascal | Pa | |
| 1 standard atmosphere | ||
| Standard acceleration due to gravity | ||
| 1 electron volt | eV | |
| Wavelength of 1 eV photon |
Trigonometrical identities
In a triangle ABC,
and
Prefixes
| Prefix | Name | Factor |
|---|---|---|
| T | tera | |
| G | giga | |
| M | mega | |
| k | kilo | |
| c | centi | |
| m | milli | |
| micro | ||
| n | nano | |
| p | pico | |
| f | femto |
Source note: The common table prints and . The 2025 question14/key15 use 9.81 and key7 uses 6371 km; those original exam values are preserved separately.
Условие
Which of the following statements are true about a cluster of main sequence stars:
- A: For two star clusters of the same total mass, the one with the larger number of stars will be brighter as measured by luminosity per unit mass.
- B: The main-sequence turnoff point for star clusters is at higher temperatures if they are older.
- C: The main-sequence turnoff point for star clusters is at lower luminosities if they are older.
Assume the mass-luminosity relationship for main-sequence stars.
(a) A and C
(b) A only
(c) C only
(d) A, B, and C
(e) A and B
Отговори
- C
Решение
A is false. The luminosity per unit mass is proportional to with our given relationship (generally, where ). Thus this value will be larger when there are fewer large stars, as opposes to many smaller stars.
B is false. The turnoff point for star clusters is at higher temperatures if they are younger. High temperature main sequence stars are usually short lived stars and thus will not exist in an old star cluster.
C is true. Low luminosity stars are usually long lived main sequence stars and thus will still exist in an old star cluster.
Answer: C
Теми и трудност
Оценена трудност: 2/5.
Звезди · Светлина и астрономически измервания · Звездна еволюция · Диаграма на Херцшпрунг–Ръсел · Поток и светимост
Предпоставки: Гимназиална подготовка, Разширена олимпиадна подготовка
Оригинал в Архива: exam_2025.pdf · официални решения: sol_2025.pdf · допълнителни данни: physical-constants.pdf