IAO 2014, Теория, Група α — Задача 6. Brightest stars
XIX International Astronomy Olympiad. Theoretical round. Group α · 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
Which four stars will be the brightest in the night sky of Cholpon-Ata in the CL (150th) century AD? Consider that ~5° of the sky above the horizon are blocked by mountains. Explain your answer and prove it by necessary drawings and calculations. Any names of stars write in Latin.
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
Due to precession of the Earth’s axis, the North celestial pole moves in a circle around the North ecliptic pole, making one circle approximately every ~26000 years (the value can be clearly seen in the sky map of precession). The time till the CL century AD is approximately half of this period, and the North pole will change its position by approximately in the direction of the brightest star in Draco constellation, γ Dra or Eltamin (in Draco the order of α-β-γ… is not the traditional one that starts from the brightest star, this fact is also clearly seen from the supplement materials). That is, in the CL century the visible part of the celestial sphere will be shifted about 47° in the direction to about the current 18h RA.
Let us list the brightest stars (for example, twice more of them than the required four) and see whether they may be seen in Cholpon-Ata in the CL century. Now we can see stars with for any RA. After 13000 years the limit will move, for RA6h and for RA18h (according to current coordinates). The situation is more complicated for other right ascensions. Anyway, the center of invisible area of the sky will be at the point (6h,−43°) and its radius will be . By easy drawing we can find that
| Star | Designation | RA | Dec | Magnitude | Vis XXI | Vis CL |
|---|---|---|---|---|---|---|
| Sirius | α CMa | 06h45m09s | −16°42′58″ | −1.46 | + | − |
| Canopus | α Car | 06h23m57s | −52°41′45″ | −0.72 | − | − |
| Toliman | α Cen | 14h39m36s | −60°50′07″ | −0.29 | − | + |
| Arcturus | α Boo | 14h15m38s | 19°10′57″ | −0.04ᵛ | + | + |
| Vega | α Lyr | 18h36m56s | 38°47′01″ | 0.03 | + | + |
| Capella | α Aur | 05h16m41s | 45°59′53″ | 0.08 | + | + |
| Rigel | β Ori | 05h14m32s | −08°12′06″ | 0.12 | + | − |
| Procyon | α CMi | 07h39m18s | 05°13′30″ | 0.38 | + | − |
That is, we will lose from the visible stars Sirius, Procyon and Rigel, and get α Centauri. The four brightest stars in the night sky of Cholpon-Ata in the CL century AD are: α Centauri, Arcturus, Vega and Capella.
Official grading criteria
- Understanding nature, precession — 1.5 pt.
- Position of North celestial pole after 13000 years — 1 pt.
- Region of sky never rising above mountains — 1.5 pt.
- Speculation about Sirius, Canopus, Toliman, Arcturus, Vega, Capella — 3 pt.
- Final correct answer — 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 |
Теми и трудност
Трудност: неоценена.
Небесна сфера и сферична астрономия · Прецесия и нутация · Небесни координати
Оригинал в Архива: alphatheo.pdf · официални решения: theosol.pdf · допълнителни данни: theocriteria.pdf · допълнителни данни: sombrero.pdf · допълнителни данни: constants.pdf · допълнителни данни: hrd.pdf