“USAAAO2019”的版本间的差异

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=== 初赛 ===
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==预赛==
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[[2019年USAAAO预赛选择题]]
  
==== 英文题目 ====
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== 决赛 ==
Time Limit: 75 Minutes
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[[2019年USAAAO决赛第1题]]
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[[2019年USAAAO决赛第2题]]
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[[2019年USAAAO决赛第3题]]
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[[2019年USAAAO决赛第4题]]
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[[2019年USAAAO决赛第5题]]
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[[2019年USAAAO决赛第6题]]
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[[2019年USAAAO决赛第7题]]
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[[2019年USAAAO决赛第8题]]
  
1. (1 point) Which of the following relates the intrinsic luminosity of a spiral galaxy with its asymptotic rotation velocity?
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==相关链接==
 
 
A. The Fundamental Plane
 
 
 
B. The Tully-Fisher Relation
 
 
 
C. The Press-Schechter Formalism
 
 
 
D. The Faber-Jackson Relation
 
 
 
 
 
2. (1 point) Which of the following correctly gives the location of Population I vs. Population II stars in the Milky Way?
 
 
 
A. Population I - Thin Disk, Spiral Arms; Population II - Halo, Bulge
 
 
 
B. Population I - Thin Disk, Bulge; Population II - Spiral Arms, Halo
 
 
 
C. Population I - Halo, Bulge; Population II - Thin Disk, Spiral Arms
 
 
 
D. Population I - Halo, Thin Disk; Population II - Bulge, Spiral Arms
 
 
 
 
 
3. (1 point) A quasar with a bolometric flux of approximately 10−12 erg s−1 cm−2 is observed at a redshift of 1.5, i.e. its comoving radial distance is about 4.4 Gpc. What is the bolometric luminosity of the quasar?
 
 
 
A. 6.0 ·1011 L B. 3.8 ·1012 L �C. 2.4 ·1013 L �D. 6.3 ·1014 L�
 
 
 
 
 
4. (1 point) Now, let’s assume that the quasar in the previous question is observed to have a companion galaxy which is 5 arcseconds apart. What is the projected linear separation of the companion galaxy from the quasar?
 
 
 
A. 107 kpc B. 29 kpc C. 74 kpc D. 43 kpc
 
 
 
 
 
5. (1 point) An observer is standing atop the Burj Khalifa, the tallest building on earth (height = 830m, latitude = 25.2N, longitude = 55.3E). Which of the following options is the closest to the shortest and longest shadow on the ground at the local noon time due to the building in a given year?
 
 
 
A. 10m, 1050m B. 25m, 950m C. 35m, 850m D. 45m, 750m
 
 
 
 
 
6. (1 point) Which of the following is closest to the ratio of the farthest distance to the horizon that can be seen by an observer standing top of the Mount Everest on Earth (height = 8.8 km) and Olympus Mons on Mars (height = 25 km)?
 
 
 
A. 0.1 B. 1 C. 5 D. 10
 
 
 
 
 
7. (1 point) An observer measures the black-body spectrum for a variety of bodies as a function of temperature and wavelength in the long wavelength limit ( hc λ � kBT) and finds that his data approximately fits the relationship log(I) = a+b log(T)+c log(λ)). Here, I is the spectral intensity in terms of wavelength, T is the temperature of the body and λ is the wavelength. Which of the following are the expected values of b and c?
 
 
 
A. 1,-4 B. 1,4 C. 4,1 D. -4,1
 
 
 
 
 
8. (1 point) Suppose a spacecraft were orbiting in a low Earth orbit at an altitude of 400 km. The spacecraft makes a single orbital maneuver to place it into a Mars transfer orbit. Delta-v (∆v) refers to the change in velocity during an orbital maneuver. What is the ∆v required for this trans-Mars injection? The semimajor axes of the orbits of Earth and Mars are 1.496 × 108 km and 2.279 × 108 km, respectively.
 
 
 
A. 2.94 km/s B. 3.57 km/s C. 6.12 km/s D. 10.85 km/s E. 11.24 km/s
 
 
 
 
 
9. (1 point) After entering Mars orbit, the spacecraft finds that over the course of the martian year, the position of Star A varies by 613.7 milliarcseconds (mas) due to the movement of the spacecraft around the sun. Determine the distance to Star A.
 
 
 
A. 1.629 pc B. 2.482 pc C. 3.259 pc D. 4.965 pc E. 6.518 pc
 
 
 
 
 
10. (1 point) Star A, of mass 3.5 M�, shows radial velocity variations 24.2 m/s in amplitude and 23.22 years in period, suggesting the presence of an orbiting exoplanet. Which of the following is closest to the mass of the exoplanet in terms of Jupiter’s masses (MJ )? Assume the exoplanet’s orbit is circular and has inclination 90◦ . The mass of Jupiter is 1.898 × 1027 kg. Assume the mass of the planet is much smaller than that of Star A.
 
 
 
A. 0.7 MJ B. 2.1 MJ C. 5.6 MJ D. 9.9 MJ E. 13.2 MJ
 
 
 
 
 
11. (1 point) Whether or not a diffraction-limited optical system is able to resolve two points as distinct can be determined by the Rayleigh criterion. β Pictoris b is one of the first exoplanets discovered using direct imaging. The star system is located 19.44 pc away, and β Pictoris b is located 9.2 AU from the host star. When viewing in infrared (λ = 1650 nm), what is the minimum telescope diameter that is able to resolve β Pictoris and its exoplanet under the Rayleigh criterion?
 
 
 
A. 0.719 m B. 0.877 m C. 1.142 m D. 1.438 m E. 1.755 m
 
 
 
 
 
12. (1 point) The celestial coordinates of the Orion Nebula are RA 05h35m, dec − 05◦230 . Which of the following is closest to the time (local solar time) when the Orion Nebula would cross the meridian on the night of February 1st 2019? The date of the vernal equinox of 2019 is March 20th.
 
 
 
A. 08:40 PM B. 10:22 PM C. 12:00 AM D. 01:38 AM E. 03:20 AM
 
 
 
 
 
13. (1 point) A yellow hypergiant located 1.04 kpc away has an apparent visual magnitude of 1.49 and a B − V color excess of 0.29. Assuming RV , the ratio of V -band extinction to B − V color excess, is 3.1, determine the absolute visual magnitude of the star.
 
 
 
A. -9.5 B. -8.9 C. -8.6 D. -8.3 E. -7.7
 
 
 
 
 
14. (1 point) The pp chain is a primary energy generation mechanism in the Sun. Each run of the process 2H + e → D + ν releases 26.73 MeV of energy. Calculate the neutrino flux on the surface of Mars (in neutrinos per m2 ), assuming that the pp chain is responsible for 100% of the Sun’s energy generation. (Mars is at a distance of 1.52 AU)
 
 
 
A. 2.54 × 1013 B. 3.17 × 1016 C. 1.37 × 1014 D. 5.94 × 1012 E. 4.45 × 1015
 
 
 
 
 
15. (1 point) A relation between which of the following pairs of properties of Cepheids variables makes Cepheids variables, specifically, useful objects for determining stellar distances?
 
 
 
A. Mass and Temperature
 
 
 
B. Period and Luminosity
 
 
 
C. Temperature and Period 
 
 
 
D. Mass and Luminosity
 
 
 
E. Period and Radius
 
 
 
 
 
16. (1 point) Assuming that the Chandrasekhar Limit is 1.4 Solar masses, estimate the maximum average density (in kg/m3 ) of a Chandrashekhar mass black hole.
 
 
 
A. 1.5 × 1022 B. 4.7 × 1014 C. 8.2 × 1010 D. 9.4 × 1018 E. 7.1 × 1026
 
 
 
 
 
17. (1 point) The Sun’s differential rotation can be estimated with the equation ω = X+Y sin2 (φ)+ Zsin4 (φ), where ω is the angular velocity in degrees per day, φ is solar latitude, and X, Y , and Z are constants (equal to 15, -2.5, and -2 degrees per day respectively). Two sunspots are spotted along the same solar meridian, one at 0◦ and the other at 40◦ . Assuming that the sunspots do not disappear or change latitude and move with the same velocity as the surface of the sun, after how many days will the sunspots be aligned once again? Round your answer to the nearest day.
 
 
 
A. 142 B. 202 C. 262 D. 312 E. 372
 
 
 
 
 
18. (1 point) An observer generates a light curve of a binary system, and notices two different minima that repeat periodically (in an alternating fashion). The time between when the light curve reaches the first minima and the second minima is 285.7 days. In solar masses, estimate the total mass of the binary system if the two stellar bodies are separated by a mean distance of 4.1 AU.
 
 
 
A. 0.0002 B. 0.0008 C. 28 D. 56 E. 112
 
 
 
 
 
19. (1 point) Eltanin, the brightest star in Draco, has the approximate coordinates RA: 17h 56m, Dec: +51.5◦ . Given that at the observer’s location, the latitude is +50◦ and the local sidereal time is 14:00, how far above the horizon will Eltanin appear? Round your answer to the nearest degree.
 
 
 
A. 26 B. 54 C. 59 D. 89 E. The star is below the horizon
 
 
 
 
 
20. (1 point) Stellar bodies located in the top left of a Hertzsprung-Russell diagram necessarily have which properties?
 
 
 
A. Low absolute magnitude, Low effective temperature
 
 
 
B. Low absolute magnitude, High effective temperature
 
 
 
C. High absolute magnitude, High effective temperature
 
 
 
D. High absolute magnitude, Low effective temperature
 
 
 
E. Intermediate absolute magnitude, Intermediate effective temperature
 
 
 
 
 
21. (1 point) Which of the following correctly orders the following distance indicators from the smallest to largest scale?
 
 
 
A. Stellar parallax, spectroscopic parallax, RR Lyrae variables, Hubble constant
 
 
 
B. Spectroscopic parallax, stellar parallax, RR Lyrae variables, Hubble constant
 
 
 
C. Stellar parallax, RR Lyrae variables, spectroscopic parallax, Hubble constant
 
 
 
D. Stellar parallax, spectroscopic parallax, Hubble constant, RR Lyrae variables
 
 
 
E. Spectroscopic parallax, stellar parallax, Hubble constant, RR Lyrae variables
 
 
 
 
 
22. (1 point) As seen from Mars, what phase will Earth appear to be in when Mars is at quadrature from Earth?
 
 
 
A. New B. Crescent C. Quarter D. Gibbous E. Full
 
 
 
 
 
23. (1 point) Which of the following stars is almost always never visible to observers in the Northern hemisphere?
 
 
 
A. Alpha Aurigae B. Gamma Cygni C. Alpha Lyrae D. Sigma Octantis E. Beta Orionis
 
 
 
 
 
24. (1 point) Two amateur astronomers A and B living in Ecuador are standing on the Equator at the Galapagos Islands (height 0 m, longitude 91◦ W) and Volcan Cayambe (height 5790 m, longitude 78◦ W) respectively. What are the differences (in degrees) of the altitudes from the horizon and zenith distances of the Sun measured by these two astronomers on March 20, 2019 when it is local noon for observer B? Neglect refraction and give your answer to the nearest degree.
 
 
 
A. Difference in altitudes: 15, Difference in zenith distances: 13.
 
 
 
B. Difference in altitudes: 13, Difference in zenith distances: 13.
 
 
 
C. Difference in altitudes: 13, Difference in zenith distances: 15. 
 
 
 
D. Difference in altitudes: 11, Difference in zenith distances: 13.
 
 
 
 
 
25. (1 point) The spectra of two stars A and B peak at wavelengths 500 nm and 250 nm respectively. What is the ratio of their luminosities if they form black holes with Schwarzschild radii in the ratio 8:1? Assume that their densities were uniform and identical before they collapsed to form a black holes and that they did not lose any mass while forming the black holes.
 
 
 
A. 2:1 B. 4:1 C. 1:4 D. 1:2
 
 
 
 
 
26. (1 point) Two stationary observers at a distance 100 AU from the sun observe transits of Mercury across the diameter of the Sun’s disk when Mercury is at perihelion and aphelion respectively. Which of the following is closest to the ratio of the aphelion transit time to the perihelion transit time? You are given that the semi-major axis and eccentricity of Mercury’s orbit are 0.387 AU and 0.21 respectively.
 
 
 
A. 1:1 B. 2:1 C. 4:1 D. 8:1
 
 
 
 
 
27. (1 point) Find the total sum of the binary system of the star Capella, if semi-major axis between them is 0.85 AU, and period of 0.285 years.
 
 
 
A. 5.5 solar masses B. 6.5 solar masses C. 7.6 solar masses D. 8.5 solar masses E. 9.5 solar masses
 
 
 
 
 
28. (1 point) The New Horizons spacecraft completed a flyby of 2014 MU69 on New Year’s day of this year. 2014 MU69 is a Kuiper Belt Object with a semi-major axis of 44.58 AU. Estimate the maximum temperature at the surface of 2014 MU69, in Kelvin, assuming the object has zero albedo.
 
 
 
A. 41.7 Kelvin B. 58.9 Kelvin C. 83.3 Kelvin D. 117.9 Kelvin
 
 
 
 
 
29. (1 point) HD 209458b is an extrasolar gas giant planet with a radius of 1.38 Jupiter radii and a mass of 0.69 Jupiter masses (1 Jupiter radius = 6.99·107 m, 1 Jupiter mass = 1.90·1027 kg). Which of the following is closest to the pressure at the very center of HD 209458b, in bars?
 
 
 
A. 109 bars B. 106 bars C. 105 bars D. 103 bars
 
 
 
 
 
30. (1 point) Imagine that our Sun was suddenly replaced by an M-dwarf with a mass half that of the Sun. If our Earth kept the same semi-major axis during this change, what would Earth’s new orbital period be around the M-dwarf?
 
 
 
A. 0.707 years B. 1 year C. 1.414 years D. 2 years
 
 
 
==== 中文题目 ====
 
欠缺
 
 
 
==== 解答 ====
 
BABDB BABDC BAACB DCCBB ACDDC BCBBC
 
 
 
=== 决赛 ===
 
  
 
==== 英文题目 ====
 
==== 英文题目 ====

2019年11月8日 (五) 21:50的版本

预赛

2019年USAAAO预赛选择题

决赛

2019年USAAAO决赛第1题 2019年USAAAO决赛第2题 2019年USAAAO决赛第3题 2019年USAAAO决赛第4题 2019年USAAAO决赛第5题 2019年USAAAO决赛第6题 2019年USAAAO决赛第7题 2019年USAAAO决赛第8题

相关链接

英文题目

The maximum score is 153 points. The test must be completed within 2.5 hours (150 minutes).

短问题

1. (7 points) Assuming that the present density of baryonic matter is ρb0 = 4.17*10^28 kg/m3 , what was the density of baryonic matter at the time of Big Bang nucelosynthesis (when T = 10^10 K)? Assume the present temperature, T0 to be 2.7 K.

2. (7 points) On the night of January 21st, 2019, there was a total lunar eclipse during a supermoon. At the time, the moon was close to perigee, at a distance of 351837 km from the earth, which was 1.4721*10^8 km from the sun. The gamma (γ) of a lunar eclipse refers to the closest distance between the center of the moon and the center of the shadow, expressed as a fraction of the earth’s radius. For this eclipse, γ = 0.3684. Given this information, find the closest estimate for the duration of totality of the eclipse.

3. (7 points) You are in the northern hemisphere and are observing rise of star A with declination δ = -8 degrees , and at the same time a star B with declination δ = +16 degrees is setting. What will happen first: next setting of the star A or rising of the star B?

4. (7 points) Consider a star with mass M and radius R. The star’s density varies as a function of radius r according to the equation ρ(r) = ρ(center)(1-sqrt(r/R)), where ρcenter is the density at the center of the star. Derive an expression for dP{dr in terms of G, M, R, and r, where P is the pressure at a given radius r.

中问题

5. (15 points) An alien spaceship from the planet Kepler 62f is in search of a rocky planet for a remote base. They’re attracted to Earth because of a fortunate coincidence: its axis of rotation points directly at their home planet. That means they can have uninterrupted communication with home by planting fixed transmitters on The North Pole. But first, they need to find out if Earth’s axis will always point in the same direction or if it undergoes precession. They can’t know without years of observation, so they hope that we, its now-extinct intelligence, have left behind the answer. While orbiting Earth, they see a few remarkable structures, including the Hoover Dam in Nevada. Zooming in on the dam, a colorful plaza with peculiar markings on its floor catches their attention. Descending on the plaza, they realize the markings are a map of the sky when the dam was built, left to indicate the date to posterity. Figure 1 is an overhead architectural map of this plaza. The center-point depicts the north ecliptic pole, and the large circle represents the path of the Earth’s axis throughout its counter-clockwise procession. As they interpret the map, they’re dismayed to realize that their star has not been and will not be Earth’s north star for very long.

Figure 1: Overhead architectural plan of the Hoover Dam plaza depicting Polaris as north star

For the purpose of this question, assume that the Earth’s axial tilt is a constant i = 23.5 degrees and its axis precesses at a constant rate.

a) Using the values on the map, and knowing that the aliens used carbon-aging to determine that the dam is 12,000 years old, find all possible values for the period of Earth’s axial precession.

b) Using the most optimistic answer (longest period) from part (a), calculate how many arcseconds the Earth’s axis precesses each day. Use the period you calculate here in the next two sections.

c) If they hadn’t been lucky enough to come across the star map and decided to build a radio interferometer to observe the movement of the celestial pole over the course of 30 days instead, how many kilometers would the baseline of their telescope array have to be, assuming it operated at a 20cm wavelength?

d) As a last resort, to keep Earth’s axis fixed, the aliens decide to counter the forces that cause the Earth’s precession by building giant nuclear thrusters on the Earth’s surface. Assume Earth’s precession is caused by external forces alone and calculate the average force (in kN) that a strategically positioned thruster would have to exert to counter them.


6. (15 points)

Figure 2 shows a full-phase light curve (“phase curve”) of the exoplanet HD 189733b taken by the Spitzer space telescope.

Use this figure to answer the following questions.

The star HD 189733 has an effective temperature of 4785 K and a radius of 0.805 Solar radii.

a) Use the depth of the planet’s transit to estimate the radius of HD 189733b, in Jupiter radii.

b) Use the depth of the eclipse of the planet by the host star to estimate the ratio of the flux of the planet HD 189733b to that of the host star HD 189733.

c) HD 189733b is so close-in to its host star that it is expected to be tidally locked. Use the phase curve to estimate the ratio of the dayside flux emitted by the planet to the nightside flux emitted by the planet.

d) This phase curve also noticeably has a phase curve offset, that is, the maximum in planet and star flux does not occur exactly at secondary eclipse. What process that occurs in a planetary atmosphere could cause such a phase curve offset?


7. (15 points)

a) Mass-Radius Relation Stellar physics often involves guessing the equation of state for stars, which is typically a relation between the pressure P and the density ρ. A family of such guesses are known as polytopes and go as follows

P = K*ρ^γ (1)

where K is a constant and the exponent γ is fixed to match a certain pressure and core temperature of a star. Given this, show that one can obtain a crude power-law scaling between the mass M of a polytopic star and its radius R of the form M9Rα. Find the exponent α for polytopic stars (justify all steps in your argument). Also, indicate the exponent γ for which the mass is independent of the radius R. Bonus: Why is this case interesting?

b) Black Holes as Blackbodies The mass radius relation for ideal non-rotating, uncharged black holes is known from relativity to be

R = 2GM/c^2 (2)

Moreover, Stephen Hawking showed that a black hole behaves like a blackbody, where its temperature (known as the Hawking temperature) is given by

T = ħc^3/8πkGM (3)

Given this information, show that the lifetime of a black hole (justify this phrase!) t ˚ scales with its mass M as

t* is proportional to Mβ (4)

where you should find the exponent β

c) Minimal Black Holes Using the information of the previous part, and Wien’s displacement law, estimate the smallest possible mass of a black hole. State any possible flaws with this estimate.

8. (15 points) In a rather weird universe, the gravitational constant G varies as a function of the scale factor aptq. G “ G0fpaq (5) Consider the model fpaq “ e bpa´1q where b “ 2.09. a) Assuming that the universe is flat, dark energy is absent, and the only constituent is matter, estimate the present age of this weird universe according to this model. Assume that the Friedmann equation: Hpaq 2 “ H2 0 pΩm ` Ωr ` Ωk ` ΩΛq (6) still holds in this setting. b) What is the behaviour of the age of the universe t as the scale factor aptq Ñ 8 ? Note that all parameters with subscript 0 indicate their present value. Take the value of Hubble’s constant as H0 “ 67.8 kms´1Mpc´1 Hint: You might need the following integrals ż 8 0 x 2 e ´x 2 dx “ ? π 4 ż 1 0 x 2 e ´x 2 dx « 0.189471 (7) 9. (15 points) a) Find the shortest distance from Boston (42.36010 N, 71.05890 W) to Beijing (39.90420 N, 116.40740 E)traveling along the Earth’s surface. Assume that the Earth is a uniform sphere of radius 6371 km. b) What fraction of the path lies within the Arctic circle (north of 66.56080 N)?

长问题