APAO 2014, Теория, Група β — Задача 2. LSVT and babr

X Asian-Pacific Astronomy Olympiad — Theoretical round · Group β · 24 ноември 2014 г.

Бележка

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.

Parameters of orbits and physical characteristics

Parameters of orbits and physical characteristics of planets, Sun and Moon.

Body	Average distance to central body (astr. units)	Average distance (million km)	Sidereal (or analogous) period (tropical years)	Period (days)	Eccentricity
Sun	$1.6\cdot10^9$	$2.5\cdot10^{11}$	$2.2\cdot10^8$	$8\cdot10^{10}$
Mercury	0.387	57.9	0.241	87.969	0.206
Venus	0.723	108.2	0.615	224.701	0.007
Earth	1.000	149.6	1.000	365.256	0.017
Moon	0.00257	0.38440	0.0748	27.3217	0.055
Mars	1.524	227.9	1.880	686.980	0.093
Jupiter	5.204	778.6	11.862	4332.59	0.048
Saturn	9.584	1433.7	29.458	10759.20	0.054
Uranus	19.191	2871.0	84.015	30685.93	0.046
Neptune	30.071	4498.6	164.778	60187.64	0.008

Body	Equatorial diameter (km)	Mass ($10^{24}$ kg)	Average density (g/cm³)	Gravity at surface (m/s²)	Maximum magnitude from Earth**	Albedo
Sun	1392000	1989000	1.409		−26.8
Mercury	4879	0.3302	5.43	3.70	−2.2	0.06
Venus	12104	4.8690	5.24	8.87	−4.7	0.78
Earth	12756	5.9742	5.515	9.81		0.36
Moon	3475	0.0735	3.34	1.62	−12.7	0.07
Mars	6794	0.6419	3.94	3.71	−2.0	0.15
Jupiter	142984	1899.8	1.33	24.86	−2.7	0.66
Saturn	120536	568.50	0.70	10.41	0.7	0.68
Uranus	51118	86.625	1.30	8.44	5.5	0.74
Neptune	49532	102.78	1.76	11.20	7.8	0.58

**) For outer planets and Moon — in mean opposition.

Coordinates	Irkutsk	Listvyanka
Longitude $\lambda$ (E)	$104^\circ18'$	$104^\circ53'$
Latitude $\varphi$ (N)	$52^\circ17'$	$51^\circ51'$
Distance to the center of the Earth	$R_I=6365.3$ km	$R_L=6365.4$ km
Timezone	UT+8	UT+8

Some constants and formulae

Constant or formula	Value
Speed of light in vacuum, $c$ (m/s)	299792458
Constant of gravitation, $G$ (N·m²/kg²)	$6.674\cdot10^{-11}$
Solar constant, $A$ (W/m²)	1367
Hubble parameter, $H_0$ (km/s/Mpc), mean value	68
Hubble parameter, diapason of values	50–100
Planck constant, $h$ (J·s)	$6.626\cdot10^{-34}$
Charge of electron, $e$ (C)	$1.602\cdot10^{-19}$
Mass of electron, $m_e$ (kg)	$9.109\cdot10^{-31}$
Proton-to-electron ratio	1836.15
Faraday constant, $F$ (C/mol)	96485
Magnetic constant, $\mu_0$ (H/m)	$1.257\cdot10^{-6}$
Universal gas constant, $R$ (J/mol/K)	8.314
Boltzmann constant, $k$ (J/K)	$1.381\cdot10^{-23}$
Stefan-Boltzmann constant, $\sigma$ (W/m²/K⁴)	$5.670\cdot10^{-8}$
Wien's displacement constant, $b$ (m·K)	0.002897
Laboratory wavelength of Hα (Å)	6562.81
Tropical year length, $T$ (days)	365.242199
Standard atmosphere (Pa)	101325
Visible light extinction by the terrestrial atmosphere in zenith (minimum)	19%, 0.23 mag
Height of homogeneous atmosphere (m)	7991
Refractive index of water for 20°C, $n$	1.334
Moment of inertia of a solid ball	$I=\frac25MR^2$
Volume of a ball	$V=\frac43\pi R^3$
Area of a sphere	$S=4\pi R^2$
$\pi$	3.14159265
e	2.71828183
Golden ratio, $\varphi$	1.61803399

Условие

The Large Solar Vacuum Telescope (LSVT) of the Institute of Solar-Terrestrial Physics, located in Listvyanka, has the main mirror 760 mm in diameter and focal length 40 m. One of the main activities of the scientists observing with the LSVT is the research of active features in solar atmosphere. Scientists regularly observe sunspots.

2.1 Draw in real scale a picture of image of the sunspot “footstep of babr” (see picture and condition of the previous problem) obtained in the focal plane of the LSVT.

2.2 When observing the Sun during sunset scientists have seen a running animal on the hill on the opposite side of the Angara river (approximately 5 km away). Scientists have suggested it is a babr, cat’s like animal (felidae) about the size of a tiger. Estimate how far you need to move the screen on which the Sun was recorded to clearly see on it the silhouette image of the animal.

2.3 Draw in actual scale in your notebook something (a point, spot, silhouette, image or something else) that will be visible on the screen.

2.4 Will the resolving power of LSVT be enough to understand what kind of animal is observed? («да-yes» or «нет-no»).

Решение

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Оригинал в Архива: betatheo.pdf · допълнителни данни: data1.pdf · допълнителни данни: data2.pdf