... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

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... Re denotes Earth radius. ... You note that the Earth orbits around the Sun in a counterclockwise direction. ... 7] In one of the eclipses of 1999 the Moon is unable to cover the entire Sun. ... Take the radius of the Earth's orbit as 300 million km, the velocity of light as 300,000 km/sec. ... 10] Section #8b, about using a total solar eclipse to estimate the distance of the Moon, includes a map of the eclipse of August 11, 1999. ... A spaceship has just enough velocity to escape the Earth's gravity...

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• Geostationary orbit and s/c [Oulu]
• Vectors
• Parallax

... satvelsrc computes as a function of time the component of the spacecraft velocity vector in the direction of given celestial source. ... SAS_ODF . or named via the generic command line parameters -o or -odfdir (see taskmain for details). ... The source coordinates obtained from the ODF can be overridden with the command line paramters withsrccoord=yes srcra=<ra> srcdec=<dec> and withorthosrc=yes defines a fictitious source in the direction perpendicular to the orbital plane. ...

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Peremennye Zvezdy", . ... Star Name: . GSC 3710-00312, USNO-A2.0 1425-04252279 . ... Variability type: . ... USNO-A2.0 1425-04252279 is located at the distance of 15?.7 from the X-ray source 1RXS J031707.9+572942, which is larger than the position error of the source (12?), but its hardness ratio HR1 = 0.03 0.29, typical of chromospherically active stars, and its character of variability allow us to assume that the star is related to the X-ray source. ... Eclipsing variability . Sine wave 1 . ...

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• Shadow Cone of a Total Solar Eclipse
• A Gegenschein Lunar Eclipse
• Eclipse Shadow Cone Over Patagonia

... Initial mass function and binary stars . ... The principal goal of this study is to show that the real shape of the initial mass function for low- and intermediate-mass stars differs from the observed one. In particular, comparison of radii of eclipsing binary components and single stars shows a noticeable difference for B0V-G0V components of eclipsing binaries and single stars of the corresponding spectral type. ...

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... You note that the Earth orbits around the Sun in a counterclockwise direction. ... 7] In one of the eclipses of 1999 the Moon is unable to cover the entire Sun. ... If an object were to be placed in the Earth orbit but with no velocity relative to the Sun, it would fall sunward. ... You may assume that the width of the Earth is 3.5 times that of the Moon (see problem 15), that the Moon is 60 Earth radii from the center of Earth and that, as seen from Earth, it is equal in size to the Sun. ...

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• How Distant is the Moon?--lesson plan #14
• Kepler's Third Law
• Estimating the Moon's Distance

... Proximity e#ects of com­ ponents (reflection of radiation and surface gravity darkening) are taken into account. ... As an example, we consider the Algol (# Persei) system, where an eclipsing pair (Algol A­B) is accompanied by the third component (Algol C). ... The surface temperature distribution for Algol A­B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation e#ect. ... We solve this equation by the iterative Newton­Raphson method. ...

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... This year's eclipse is unique in duration. ... Although, at the present time, there are 6 solar observatories belonging to leading space agencies in orbit around the Earth, the eclipse of 22 July, 2009, will only be seen by two of them: the Russian CORONAS-PHOTON satellite equipped with TESIS telescopes and Japan's HINODE satellite fitted with an XRT space telescope. ... TESIS will be the first of the two devices (and the very first on Earth) to witness the solar eclipse. ...

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• The culmination of the solar eclipse coincided with the strongest magnetic
• The X-ray Solar Eclipse
• Solar eclipse - the eighth wonder of the world - TESIS photo gallery

... A light curve decomposition tool ( LFIT ) developed by Keith Horne and Tom Marsh and its application on HST-data of the eclipsing dwarf nova IP Peg will be presented. ... Our LFIT code decomposes time-resolved spectral data into N components with parameterized light curve shapes, solving for the spectra of each component. ... To apply this algorithm to the HST and UBVRI eclipses of IP Peg, we add an ellipsoidal light curve for the companion star, and a more detailed description of the bright spot. ...

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• HST Spectral Maps of Accretion Disks in Cataclysmic Binaries
• The Spectroscopic Orbit of the Evolved Binary HD 197770
• STScI Preprint #1207

HD185510 (=V1379 Aql) is an eclipsing double-lined RS CVn binary containing a K0 III/IV giant and a hot subluminous companion. ... This was sufficient to resolve all four times of contact and, with data from previous work on this system, to derive a solution for the absolute dimensions of the system. ... Neglecting Ly-alpha, an alternative solution of Teff=31000+/-1500 K, log g=6.5+/-0.2, and E(B-V)=0.1+/-0.03 is obtained from the orbital solution below. ...

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• Observations with the Faulkes Telescopes
• Armagh Observatory
• Lunar Eclipse March 2007

... In particular, members of the project regularly organize events dedicated to various interesting astronomical phenomena and events - solar and lunar eclipses, transit of Venus, etc. A total lunar eclipse will occur on April 15th, 2014, the first in two and half years. ... GLORIA will travel to Peru to broadcast the event live. ... Lunar eclipse . Lunar eclipses occur when the Moon passes into the Earth's shadow. ... A partial eclipse will be visible from the Canary Islands. The broadcast . ...

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• Detection of radio pulsar pairs
• Optical component of GRB080319B

MICROSATELLITE PROGRAM KOLIBRY MS MS PROGRAM PARTICIPANTS PROJECT IMPLEMENTATION . INTERNATIONAL SPACE STATION . KOLIBRY MS . The Kolibry satellite was developed as a base satellite as applied to the entire Program with respect to its characteristics: . ... Content of service systems; . ... In-flight control of its operation. ... Antenna system . ... The system of data acquisition and control; . ... Passive thermal control system; . ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• RSC "Energia" - Automatic Space Systems
• RSC "Energia" - History
• S.P. Korolev RSC Energia - International Space Station

Text of these problems is available also in other languages : . ... What can one see in the Moon's sky more often - the Sun or the Earth? ... There are about of 250 millions of stars in the elliptical galaxy M32 (a satellite of Andromeda galaxy). ... The masses of Capella's components. ... You are proposed to estimate the masses of Capella's components, using our observational data. ... A galaxy's mass. ... Estimate the mass of FGC 1908 and compare it to the mass of our galaxy. ...

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CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

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• Chapter 5. Listing of Installed Components

... 2003 January 6 . Shadow Cone of a Total Solar Eclipse . ... Explanation: Sometimes, during a total eclipse of the Sun, a strange shadow of darkness can be seen stretching off into the distance. Called a shadow cone, they are visible because the Earth's atmosphere is not completely transparent, scattering sunlight and hence appearing blue during the day. ... Visible above is a shadow cone caught during a total solar eclipse visible last month from South Australia . ... About APOD | ...

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• APOD: 2010 August 4 - Eclipse Shadow Cone Over Patagonia
• APOD: 2015 October 14 - A Gegenschein Lunar Eclipse
• APOD: 2005 April 23 - Eclipsed Moon in Infrared

... In this section, we develop a physical model of the secondary as a disk that is centrifugally supported in the radial direction and hydrostatically supported in the vertical direction. We assume that the disk is vertically isothermal and well mixed. ... where is the mean molecular mass of the gas, is the orbital period at the outer edge of the disk in years, and all of the mass of the secondary has been assumed to be concentrated near its center, so the Keplerian approximation is valid. ...

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• Characteristics of the Aurig? System
• The AstroStat Slog Blog Archive [ArXiv] component separation methods
• Eclipse Lightcurves for the Hydrostatic Model

... On the morning of Thursday, 26 February, amid the Gal pagos Islands, the Sun will fade from view. Not the culmination of ancient prophecy, but none less mystical, Earth's small Moon will be executing a slow slide past the enormous Sun. ... And anyone living in southern North America, Central America, northern South America, or on islands and cruise ships in the Caribbean Sea will, weather permitting, have the opportunity to experience the wonder of a solar eclipse. ...

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• ASP: Up, Up, and Away
• ASP: Australia?s 2002 Total Eclipse of the Sun
• ASP: Counterpoint: Where Is the Best Place to View a Solar Eclipse?

... Popper (1959) classified the eclipsing components as B8 V and B9.5 V. According to Wolff and Preston (1978) the primary component (B8) is a HgMn star. Spectroscopic elements were determined by Wyse (1936) from observations made in the years 1934 - 1935 and by Harper (1937) from observations 1935 -1936. ... Rachkovskaya (1985) according to Harper - 2.68 and 2.36 observed the star in the years 1967 -1968 and 1981 - 1982 and obtained the mass ratio q » 1. ...

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• Iron abundance in the atmospheres of components of the binary system 41...
• Parameters of the 41 Dra system components

... Gravity data reflect changes, related to the groundwater redistribution, ice melting, and precipitation accumulation. ... We apply Multichannel Singular Spectrum Analysis (MSSA, or extended EOF) technique to filter GRACE data and separate the principal components (PCs) of different periods. We performed data averaging over the large river basins of Russia. ... Fig 1. ... MSSA is a promising method for GRACE data processing, de-striping, filtering, and Principal Components (PCs) separation. ...

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• Natural Satellites Service. Mutual occultations and eclipses of the major
• jg0029
• jg0026

Next: Pass band integrations Up: Fit scenarios Previous: Triple with velocity curves Contents . Fit all three masses, as well as the inclination of one of the pairs. That not any combination of orbital inclinations is allowed can be seen from the fact that the triple consists of two double-lined binaries and only one mass solution exists for a given inclination. ... Christian Hummel 2015-04-28 ...

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• The format of STARTABLE
• How DFS components access databases
• Structural Components of a Double-Barred Spiral Galaxy | ESO