... фотометричн? характеристики планет . Планета . ... екватор?альний . ... пер?од . обертання 3 . Пер?од . ... Земля=1 . ... в?дстань . ... Венери вказана м?н?мальна геоцентрична в?дстань це в?дстань до планети п?д час нижнього сполучення; для зовн?шних планет це в?дстань п?д час протистояння. ... 8 Альбедо показу?, яку частку падаючого св?тла розс?ю? дана поверхня. 9 а.о. астроном?чна одиниця: середня в?дстань в?д Земл? до Сонця, дор?вню? 149.6 м?льйон?в км. ...

XMM­Newton CCF Release Note XMM­CCF­REL­86 EPIC MOS ASTROMETRY B. Altieri August 2, 2001 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag EMOS1 LINCOORD 0016 2000­01­01T00:00:00 FOV NO EMOS2 LINCOORD 0016 2000­01­01T00:00:00 FOV NO 2 Changes The relatove positions between CCDs for both MOS cameras have been adjusted to provide the highest astrometric accuracy over the full field­of­view of the MOS cameras. ...

F(6 cm) Other Name ct/s erg cm -2 s -1 µJy FX/FR mJy # r B R Class z Catalogs WGAJ0011.2- 3620 0.002 1.73E - 14 0.003 -12.73 96 0.12 21.3 FSRQ 2.324 WGAJ0012.5- 1629 0.097 1.28E - 12 0.29 -10.53 50 0.62 17.7 FSRQ 0.151 1 WGAJ0015.5+ 3052 0.019 2.82E - 13 0.083 -11.37 89 0.62 16.3 17.2 FSRQ 1.619 0.023 3.16E - 13 0.095 WGAJ0029.0+ 0509 0.006 6.33E - 14 0.014 -12.71 377 0.00 19.3 18.1 FSRQ 1.633 WGAJ0032.5- 2849 ...

... Name Designation ff ffi J (ffi J ) H (ffi H ) K (ffi K ) J \Gamma K H \Gamma K Nights a AS01­0 FS02 00 55 09.9 00 43 13 10.716 ( 0.005 ) 10.507 ( 0.010 ) 10.470 (0.003) 0.25 0.04 6,6,6 AS02­0 SAO054271 00 55 58.6 39 10 09 8.775 (0.006) 8.771 ( 0.012 ) 8.770 ( 0.009 ) 0.01 0.00 5,6,6 AS03­0 FS03 01 04 21.6 04 13 39 12.606 ( 0.011 ) 12.729 ( 0.008 ) 12.827 ( 0.013 ) ­0.22 ­0.10 6,6,6 AS04­0 FS04 01 54 37.6 00 43 01 10.555 (0.004) 10.301 ( ...

WGN, the Journal of the IMO XX:X (200X) 1 General Relativistic Precession in Meteoroid Orbits A. Sekhar1 ,2 1 There are only very few past works related to the application of general relativity in the orbital evolution of small solar system bodies. ... However the maximum r ( 2 в 10-3 AU (1 - e cos )2 in 1 kyr) is exhibited by Daytime Arietids due to low q The values of and r given in Table 1 and 2 and low a compounded by the favourable value in . ... It can depend on for a constant value of . ...

... Be/X-Ray Binaries and candidates in the LMC . ... This Einstein and ROSAT variable source was identified with a Be star by Schmidtke, Cowley, Frattare et al. ... This super-soft X-ray source was discovered with XMM-Newton ( Kahabka, Haberl, Payne & Filipovic (2006) ). ... The transient X-ray source RX J0529.8-6556 was detected during one single outburst as a 69.5-s X-ray pulsar by Haberl, Dennerl, Pietsch & Reinsch 1997) , who identified it with a relatively bright blue star showing weak H? emission...

... Spectral Studies of Asteroids 21 Lutetia and 4 Vesta as Objects of Space Missions V. V. Busarev Sternberg Astronomical Institute, Universitetskii pr. ... When interpreting the reflectance spectra of Lutetia and Vesta, we dis cuss the spectral classification by Tholen (1984) from the standpoint of its general importance for the estima tion of the mineralogical type of the asteroids and the study of their origin and evolution. ... It contains 14 classes of asteroids. ... 2007; Busarev, 2008) were...

. Computer Ephemeris for 2014 from DE200/LE200. Mean places of fundamental stars at J2014.5 # name m Sp paralax alpha dif mu(al) delta dif mu(dl) " h m s s s o ' " " " 902 Psc omega 4.01 F5 0.012 3.437 3.085 0.0103 65636.77 19.93 -1.15 903 Tuc epsilon 4.50 B9 0.000 39.621 3.084 0.0077 -652947.46 20.02 -0.24 904 Oct theta 4.78 K0 0.011 219.259 3.016 -0.0188 -765908.52 19.86 -1.77 1630 Psc 30 4.41 M3 0.043 242.249 3.077 0.0034 -55600.70 20.00 -0.41 905 Cet 2 4.55 A0 0.004 428.899 3.070 0.0018 -171519.15 20.03

... material . ... cryst. enstatite . n,k [tab] . ... transm. [fig] . ... ext (T) [fig] . ... em.spectra [fig] . ... n,k [fig] . ... olivine . ... Opt. 11, 142. cryst. olivine . ... refl. a,b,c [fig]; par. [tab] . ... 1974) Astrophys.J. 191, 415. cryst. olivine . ... J. 199, 660. cryst. olivine . ... Kraetschmer, Huffman (1979) Astrophys.Sp.Sci. 61, 195. cryst. olivine . ... Sci. 134, 95. cryst. olivine . ... 1998) Astrophys.J. 496, 1058. cryst. olivine . ... refl. [fig]; disp.par. [tab] . ...

This is an implementation of RD-tree data structure using GiST interface of PostgreSQL. ... desc') - sort intarray test =# select sort ('{1,2,3}':: int [],'desc'); sort --------- {3,2,1} (1 row) int [] sort ( int []) - sort in ascending order int [] sort _asc( int []), sort _desc( int []) - shortcuts for sort int [] uniq( int []) - returns unique elements test =# select uniq( sort ('{1,2,3,2,1}':: int [])); uniq --------- {1,2,3} (1 row) int idx( ...

Лекция 6. Нормальная Земля | ... 7.2 Нормальная сила тяжести . 7.3 Вторые производные гравитационного потенциала . ... Вторые производные нормального потенциала. ... В геодезии и геофизике основной характеристикой гравитационного поля являются гравитационные аномалии , полученные как разность между наблюденным значением удельной силы тяжести и предвычисленным. ... В действительности же нормальную силу тяжести относят к общему земному эллипсоиду, а наблюденное -- к физической поверхности Земли. ...

... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...

... Planets . ... Exoplanets . ... Image 1-Artists impression of an exoplanet in orbit around host star. ... Supposedly the closest exoplanet to us is also located in this system around one of the other stars, Alpha Centauri B. €аThis hot, Earth-sized, rocky exoplanet, Alpha Centauri Bb was discovered by astronomers in Geneva last year. ... The exoplanet, 55 Cancri e has almost 8 times the mass of the Earth with a diameter twice the size and is thought to be a carbon planet. ... Exoplanets Glossary | ...

... We examine the effects of amplifiers gain fluctuations, of fluctuations in the amplifiers noise temperatures, in the reference load tem­ perature and in the DC gain ratio. We find that 1=f gain fluctuations are suppressed by proper gain modulation, leaving fluctuations in the amplifiers noise temperatures as the main source of 1=f type noise. ... 4 Discussion and conclusions We have shown that the dominant source of 1=f noise in the radiometer output is amplifier noise temperature fluctuations. ...

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