OWAO 2023, Практически тур — Задача 3. Eclipse in Siberia

ΩWAO 2023 ◇ Practical Round ◇ Problems

Условие

There are two videos:

  • eclipse1.mp4 or https://youtu.be/nsWVPedsQNk
  • eclipse2.mp4 or https://youtu.be/Lw7GGm0U94g

showing conditions for the annular solar eclipse on July 25, 2120. The greatest eclipse will be observed in Siberia, geographical region in Russia. Estimate the altitude of the Sun at the point where the maximum magnitude of the eclipse will be observed (if the weather is good).

Hint: the center of lunar antumbra reaching the Earth’s surface is marked by green cross.

Schematic of a solar eclipse: the Sun on the left, a small globe in the middle casting a dark umbra cone and grey penumbra/antumbra regions to the right, bounded by red and blue tangent lines; three inset sky views labelled Penumbra (partially covered Sun), Umbra (fully covered Sun) and Antumbra (annular ring) are connected by red lines to the corresponding regions.

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})/\mathrm{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}} (bol.)
Effective temperatureT⊙=5.8⋅103 KT_{\odot} = 5.8 \cdot 10^3\ \mathrm{K}
LuminosityL⊙=3.828⋅1026 WL_{\odot} = 3.828 \cdot 10^{26}\ \mathrm{W}
Emission constants
Stefan–Boltzmannσ=5.67⋅10−8 (W/m2)/K4\sigma = 5.67 \cdot 10^{-8}\ (\mathrm{W/m^2})/\mathrm{K^4}
Wien’s displacementb=2898 μm⋅Kb = 2898\ \mu\mathrm{m} \cdot \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}
Hydrogen spectrum
Lyman Lα\alphaλLα=1215.7\lambda_{L\alpha} = 1215.7 Å
Balmer Hα\alphaλHα=6562.8\lambda_{H\alpha} = 6562.8 Å

Оригинал в Архива: OWAO_2023_Practical_Round_Problems.pdf · официални решения: OWAO_2023_Practical_Round_Solutions.pdf