RTT150, main page
RTT150
Russian-Turkish 1.5-m Telescope

 
High energy Astrophysics department of IKI, Moscow
International astrophysical observatory Spectrum-X-Gamma
International astrophysical space observatory INTEGRAL

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HEAD IKI

Astronomical calculators

Current date and time. For given geographical position shows the current local date and time, universal date and time, cuurent siderial time. Daylight savings time is also taken into account.
Calendar for a year. Shows the calendar for a given year. Source of the script: http://javascripts.boom.ru/calendar.htm, modified by N.Alexandrovich.
Universal date converter. Inputs date and time in any of 10 formats (usual date and time, decimal day, decimal number of day of year, decimal year, several types of Julian Days). Converts from any format to all the rest and shows the day of week. Direct input of current date and time in also provided, time zone correction is made.
Distance between two points. Calculates angular distance between two points on the celestial sphere with given coordinates. Accepts hh:mm:ss & o:':", decimal degrees and radians.
Source visibility for a year. For a given observing location calculates height above horizon of a source with given equatorial coordinates for every hour within a given range of dates. Also marks the dark time of night, presence of the Moon at a phase higher than specified and proximity of the Moon to the source closer than by acceptable distance.
Precession correction. Converts equatorial coordinates from one given epoch to the other and determines the constellation in which this point is located.
Universal coordinates converter. Precession correction and mutual conversion between equatorial, ecliptical and galactic coordinates. Shows all coordinates and inclination angle of ecliptics to equator for two epochs, determines the constellation.
Atmospheric refraction. Correction of source altitude and its zenith angle for atmospheric refraction. Converts astrometric position to the apparent one and vice versa.
Astrophotomery. Calculation of stellar magnitudes from flux ratio and backwards. Determining the visual and absolute magnitudes, luminocity, distance (parallax) and extinction.