IAO 2014, Теория, Група β — Задача 5. Climate
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
The XXXII (32) century AD. Due to unknown reasons, the Sun became cooler, not changing its size, and the inclination of ecliptic to the celestial equator plane decreased to zero. Scientists proved that the problem of preserving the Earth’s climate and the annual change of seasons can be solved by a small star, negligible mass, but similar to a main-sequence star, moving in a circular orbit around the Sun. The star will revolve around the Sun as an inner planet, resulting in establishing a temperature regime on the Earth similar to the actual one at Issyk-Kul: the average winter and summer temperatures are -3 and +17 degrees respectively.

5.1. Estimate the temperature of the cool Sun.
5.2. Estimate to what spectral class the star which will be placed in the desired orbit will correspond.
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
In order to get an inner orbit of the star that would provide a seasonal cycle with a periodicity of 1 year, it is necessary that its close position with the Earth would take place once a year. That is, the synodic period of its revolution should be one year. It is not difficult to find that the sidereal period of revolution of the celestial body must be equal to
and the radius of its orbit, from the III Kepler’s law:
Thus, the new celestial body will once a year become close to the Earth at a distance of au, providing summer on the planet, and once a year move away to a distance of au, leaving the Earth in winter.
The ratio of energies received by the Earth from the new star in summer and winter will be
The ratio of these energies to the energy , received from the new star at a distance of 1 au is
At the same time, the Earth will always receive additional energy from the cooler Sun, that is, in the summer, and . To keep the heat balance, all the incoming energy should be radiated.
The ratio of the energy radiated by the Earth in summer and winter will be
Neglecting the effects of delays of the seasons compared to the maxima and minima of the energy income, let us assume that , . Then we can write:
The sum of and the average for the period must be the same as the Earth receives nowadays, . To estimate the average value of , let us take , and so
5.1. Thus, the Sun in new conditions will emit 4.6% less energy, and so its temperature will be lower and equal to
5.2. To understand what spectral type will correspond to the star, we calculate by how many magnitudes it is fainter than the Sun:
From the HR diagram, we find that it is about the spectral type K3.
Source note: the winter ratio is printed with (R₀−R)² in its denominator although the preceding winter distance is R₀+R and the numerical 0.38 corresponds to the latter. The printed formula is retained. Calligraphic ℰ here represents the separate radiated-energy symbol used in the key.
Official grading criteria
- Understanding nature of the effect and conclusion synodic period is 1 year – 1 pt.
- Calculation sidereal period = 0.5 years – 1 pt.
- Radius of the orbit from the III Kepler's law – 1 pt.
- Energy balances — 2 pt.
- 5.1. Temperature of Sun — 1 pt.
- 5.2. ΔM=−(5/2)lg(0.0464)≈3.3 and from HR diagram spectral type K 3 — 2 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