IAO 2014, Теория, Група β — Задача 1. Dreams of the Polar Bear
XIX International Astronomy Olympiad. Theoretical round. Group β · 12 октомври 2014 г. · 8 т.
Бележка
General note. Maybe not all problems have correct questions. Some questions (maybe the main question of the problem, maybe one of the subquestions) may make no real sense. In this case you have to write in your answer (in English or Russian): «impossible situation – ситуация невозможна». Of course, this answer has to be explained numerically or logically.
Data from the tables (Planetary data, stars, constants, etc.) may be used for solving every problem.
The answers «Да-Yes» or «Нет-No» have to be written in English or Russian.
Условие
Terrestrial Polar Bear-observer, watching the lunar disk in the phase of the full moon, in his dreams became thousand times closer to it. What did the magnitude of the Moon become? The solution has to include an artistic picture with an image of the Bear-observer on the North Pole.
Source reference charts


Решение
Official sketches for solutions. The source notes that these sketches are not full; team leaders should give more detailed explanations, while correct student solutions sufficient for 8 points may be shorter.
Solution
It would seem that approaching 10 times closer to an object reduces its apparent magnitude by 5 magnitudes, and so approaching times closer reduces the apparent magnitude by magnitudes. The magnitude of the Moon would be equal to ?
Would it? It turns out that in this case the Moon shines 2.3 times brighter than the Sun! In fact, this cannot happen!
Actually, the rule of reducing the magnitude by 5 when approaching the object 10 times closer is valid only for point-like objects, or objects for which the small-angle approximation is acceptable, i.e., an approach 10 times closer to the object increases the apparent solid angle by a factor of 100. Indeed, the magnitude decrease of extended objects, like the lunar disc, is related to the increase of the object’s apparent solid angle while keeping brightness unchanged.
The solid angle of the visible surface of the Moon from the Earth is
When using the small-angle approximation, approaching times closer would increase the visible area by the factor of times, and it would become 67 rad². However, this solid angle cannot be larger than the solid angle of a hemisphere, . That is, in the calculations we have overestimated the area by a factor of at least , and make an error in the magnitude of at least . Thus, the magnitude of the lunar disk cannot be less than .
More precise calculations show that when approaching 1000 times closer to the surface of the Moon (approximately from 380 thousand km to 380 km), the apparent solid angle will be
i.e. it will increase by a factor of approximately and (in this model of the same brightness of the lunar surface) the magnitude is
Official grading criteria
Solution: 7 pt in total, including:
- Understanding about impossibility to use approximation of point-like objects — 3 pt.
- Result approximately Ω₂/Ω₁=40000 — 2 pt.
- Formula and final calculations −12.7−2.5log(40000)≈−24.2 — 2 pt.
For any solution based on calculations in approximation of point-like objects or any answer resulting in larger than the Sun brightness, total mark (except mark for the picture) should not be larger than 1 pt for group α or 0.5 pt for group β.
Artistic picture of the Bear — 1 pt.
Jury note: evaluate the solution in essence rather than formal presence of sentences/formulae; award points when subsequent steps de facto use the required positions.
Parameters of orbits and physical characteristics
| Body | Distance (AU) | Distance (10⁶ km) | Period (tropical years) | Period (days) | Inclination i (°) | Eccentricity | Equatorial diameter (km) | Mass (10²⁴ kg) | Density (g/cm³) | Gravity (m/s²) | Axial tilt (°) | Max. magnitude | Albedo |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Sun | 1392000 | 1989000 | 1.409 | −26.74 | |||||||||
| Mercury | 0.387 | 57.9 | 0.241 | 87.969 | 7.00 | 0.206 | 4879 | 0.3302 | 5.43 | 3.70 | 0.01 | 0.06 | |
| Venus | 0.723 | 108.2 | 0.615 | 224.7007 | 3.40 | 0.007 | 12104 | 4.8690 | 5.24 | 8.87 | 177.36 | 0.78 | |
| Earth | 1.000 | 149.6 | 1.000 | 365.2564 | 0.00 | 0.017 | 12756 | 5.9742 | 5.515 | 9.81 | 23.44 | 0.36 | |
| Moon | 0.00257 | 0.38440 | 0.0748 | 27.3217 | 5.15 | 0.055 | 3475 | 0.07348 | 3.34 | 1.62 | 6.7 | −12.7 | 0.07 |
| Mars | 1.524 | 227.9 | 1.880 | 686.98 | 1.85 | 0.093 | 6794 | 0.6419 | 3.94 | 3.71 | 25.19 | −2.0 | 0.15 |
| Jupiter | 5.204 | 778.6 | 11.862 | 4332.59 | 1.30 | 0.048 | 142984 | 1899.8 | 1.33 | 24.86 | 3.13 | −2.7 | 0.66 |
| Saturn | 9.584 | 1433.7 | 29.458 | 10759.20 | 2.48 | 0.054 | 120536 | 568.50 | 0.70 | 10.41 | 26.73 | 0.7 | 0.68 |
| Eris | 68.05 | 205029 | 43.82 | 0.435 | 2326 | 0.0167 | 2.52 | 0.7 | 0.96 |
Source footnote: for outer planets and Moon — in mean opposition. Blank cells are blank in the source.
Some constants and formulae
| Constant or formula | Value |
|---|---|
| Speed of light in vacuum c (m/s) | 299792458 |
| Constant of gravitation G (N·m²/kg²) | |
| Solar constant A (W/m²) | 1367 |
| Hubble parameter H₀ (km/s/Mpc), mean | 71 |
| Hubble parameter, range | 50–100 |
| Planck constant h (J·s) | |
| Charge of electron e (C) | |
| Mass of electron mₑ (kg) | |
| Proton-to-electron ratio | 1836.15 |
| Faraday constant F (C/mol) | 96485 |
| Magnetic constant μ₀ (H/m) | |
| Universal gas constant R (J/mol/K) | 8.314 |
| Boltzmann constant k (J/K) | |
| Stefan–Boltzmann constant σ (W/m²/K⁴) | |
| Wien displacement constant b (m·K) | 0.002897 |
| Laboratory wavelength Hα (Å) | 6562.81 |
| Tropical year length T (days) | 365.242199 |
| Standard atmosphere (Pa) | 101325 |
| Visible light extinction by terrestrial atmosphere in zenith (minimum) | 19%, 0.23 magnitudes |
| Height of homogeneous atmosphere (m) | 7991 |
| Refractive index of water for 20°C n | 1.334 |
| Moment of inertia of a solid ball | |
| Volume of a ball | |
| Area of sphere | |
| π | 3.14159265 |
| e | 2.71828183 |
| Golden ratio φ | 1.61803399 |
| Coordinates | Bishkek | Cholpon-Ata |
|---|---|---|
| Longitude E | 74°34′ | 77°05′ |
| Latitude N | 42°52′ | 42°39′ |
| Timezone | UT+6 | UT+6 |
28 brightest stars and some other stars
| Name | Designation | RA | Dec | Parallax (arcsec) | Magnitude | Spectral class |
|---|---|---|---|---|---|---|
| Altair | α Aql | 19h50m47s | 08°52′06″ | 0.195 | 0.77 | A7 |
| Capella | α Aur | 05h16m41s | 45°59′53″ | 0.073 | 0.08 | G5+G0 |
| Arcturus | α Boo | 14h15m38s | 19°10′57″ | 0.089 | −0.04ᵛ | K1 |
| Canopus | α Car | 06h23m57s | −52°41′45″ | 0.028 | −0.72 | F0 |
| Miaplacidus | β Car | 09h13m12s | −69°43′02″ | 0.029 | 1.68 | A2 |
| Toliman (Rigel Kent) | α Cen | 14h39m36s | −60°50′07″ | 0.747 | −0.01; 1.33 | G2; K1 |
| Hadar | β Cen | 14h03m49s | −60°22′23″ | 0.009 | 0.61 | B1 |
| Sirius | α CMa | 06h45m09s | −16°42′58″ | 0.375 | −1.46 | A1 |
| Adara | ε CMa | 06h58m38s | −28°58′19″ | 0.008 | 1.50 | B2 |
| Procyon | α CMi | 07h39m18s | 05°13′30″ | 0.288 | 0.38 | F5 |
| Acrux | α Cru | 12h26m36s | −63°05′57″ | 0.010 | 0.77 | B0 |
| Becrux | β Cru | 12h47m43s | −59°41′20″ | 0.009 | 1.30 | B0 |
| Gacrux | γ Cru | 12h31m10s | −57°06′48″ | 0.037 | 1.60 | M4 |
| Deneb | α Cyg | 20h41m26s | 45°16′49″ | 0.002 | 1.25 | A2 |
| Achernar | α Eri | 01h37m43s | −57°14′12″ | 0.026 | 0.46 | B3 |
| Castor | α Gem | 07h34m36s | 31°53′18″ | 0.065 | 1.58 | A1+A2 |
| Pollux | β Gem | 07h45m19s | 28°01′35″ | 0.097 | 1.14 | K0 |
| Regulus | α Leo | 10h08m22s | 11°58′02″ | 0.041 | 1.35 | B7 |
| Vega | α Lyr | 18h36m56s | 38°47′01″ | 0.123 | 0.03 | A0 |
| Betelgeuse | α Ori | 05h55m10s | 07°24′25″ | 0.005 | 0.5ᵛ | M2 |
| Rigel | β Ori | 05h14m32s | −08°12′06″ | 0.013 | 0.12 | B8 |
| Bellatrix | γ Ori | 05h25m08s | 06°20′59″ | 0.013 | 1.64 | B2 |
| Fomalhaut | α PsA | 22h57m39s | −29°37′20″ | 0.130 | 1.16 | A3 |
| Antares | α Sco | 16h29m24s | −26°25′55″ | 0.024 | 0.96 | M1+B4 |
| Shaula | λ Sco | 17h33m37s | −37°06′14″ | 0.005 | 1.62 | B2 |
| Aldebaran | α Tau | 04h35m55s | 16°30′33″ | 0.048 | 0.85ᵛ | K5 |
| Elnath | β Tau | 05h26m18s | 28°36′27″ | 0.025 | 1.66 | B7 |
| Spica | α Vir | 13h25m12s | −11°09′41″ | 0.023 | 0.98 | B1 |
Some other stars
| Name | Designation | RA | Dec | Parallax (arcsec) | Magnitude | Spectral class |
|---|---|---|---|---|---|---|
| Hamal | α Ari | 02h07m10s | 23°27′45″ | 0.050 | 2.01 | K2 |
| Sheratan | β Ari | 01h54m39s | 20°48′30″ | 0.055 | 2.64 | A5 |
| Thuban | α Dra | 14h04m23s | 64°22′33″ | 0.011 | 3.65 | A0 |
| Rastaban | β Dra | 17h30m26s | 52°18′05″ | 0.009 | 2.79 | G2 |
| Eltamin | γ Dra | 17h56m36s | 51°29′20″ | 0.021 | 2.24 | K5 |
| Polaris | α UMi | 02h31m49s | 89°15′51″ | 0.007 | 1.97ᵛ | F7 |
| Kochab | β UMi | 14h50m42s | 74°09′20″ | 0.025 | 2.07 | K4 |
| Pherkad | γ UMi | 15h20m44s | 71°50′02″ | 0.007 | 3.06ᵛ | A3 |
| Yildun | δ UMi | 17h32m19s | 86°35′11″ | 0.019 | 4.35 | A1 |
| Proxima Centauri | V645 Cen, α Cen C | 14h29m43s | −62°40′46″ | 0.769 | 11.05 | M5.5 |
Оригинал в Архива: betatheo.pdf · официални решения: theosol.pdf · допълнителни данни: theocriteria.pdf · допълнителни данни: sombrero.pdf · допълнителни данни: constants.pdf · допълнителни данни: hrd.pdf