OWAO 2022, Теория — Задача 5. Follow the Shadow

ΩWAO 2022 ◇ Theoretical Round ◇ Problems

Условие

Occultation of a star by the Moon begins on Earth at the North Pole, and ends at a point with latitude 33∘33^{\circ} North on the prime meridian (0∘0^{\circ} longitude) at 0h0^{\mathrm{h}} local time. Find the star’s equatorial coordinates and the occultation date.

Отговори

Решение

Константи
Universal
Speed of lightc=3.00⋅108 m/sc = 3.00\cdot 10^8\ \mathrm{m/s}
Planck constanth=6.63⋅10−34 J⋅sh = 6.63\cdot 10^{-34}\ \mathrm{J\cdot s}
Hubble constantH0=70 (km/s)/MpcH_0 = 70\ \mathrm{(km/s)/Mpc}
Astronomical unit1 au=149.6⋅106 km1\ \mathrm{au} = 149.6\cdot 10^6\ \mathrm{km}
Parsec1 pc=206 265 au1\ \mathrm{pc} = 206\,265\ \mathrm{au}
Earth
RadiusR⊕=6371 kmR_\oplus = 6371\ \mathrm{km}
Obliquityε=23.4∘\varepsilon = 23.4^{\circ}
Surface gravityg=9.81 m/s2g = 9.81\ \mathrm{m/s^2}
Orbital periodT⊕=365.26dT_\oplus = 365.26^{\mathrm{d}}
Orbital eccentricitye⊕=0.0167e_\oplus = 0.0167
Moon
RadiusR☾=1737 kmR_{\text{☾}} = 1737\ \mathrm{km}
Orbital periodT☾=27.32dT_{\text{☾}} = 27.32^{\mathrm{d}}
Orbital inclinationi☾=5.1∘i_{\text{☾}} = 5.1^{\circ}
Sun
RadiusR⊙=6.96⋅105 kmR_\odot = 6.96\cdot 10^5\ \mathrm{km}
Absolute magnitudeM⊙=4.74mM_\odot = 4.74^{\mathrm{m}}
Effective temperatureT⊙=5.8⋅103 KT_\odot = 5.8\cdot 10^3\ \mathrm{K}
UBV systemMean wavelengths
U bandλU=364 nm\lambda_U = 364\ \mathrm{nm}
B bandλB=442 nm\lambda_B = 442\ \mathrm{nm}
V bandλV=540 nm\lambda_V = 540\ \mathrm{nm}

Оригинал в Архива: OWAO_2022_Theoretical_Problems.pdf · официални решения: OWAO_2022_Theoretical_Solutions.pdf