en:documentation:detailed_information
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| ====== Detailed Information ====== | ====== Detailed Information ====== | ||
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| * When //edit label// mode is **on** (the {{en: | * When //edit label// mode is **on** (the {{en: | ||
| * Get a " | * Get a " | ||
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| ===== Content of the detailed information window ===== | ===== Content of the detailed information window ===== | ||
| - | In any detailed information window you can distinguish 4 paragraphs with their specific data. | + | In any detailed information window you can distinguish 4 paragraphs with their specific |
| ==== Object information and characteristics | ==== Object information and characteristics | ||
| For stars and deep sky objects, this paragraph contains static information about the object which was retrieved from the catalog. | For stars and deep sky objects, this paragraph contains static information about the object which was retrieved from the catalog. | ||
| For Solar system objects, you can find information like the object type, and the object identification (name). Please forgive SkyChart when it shows you the Sun as a planet. All other information in this paragraph is dynamically calculated from the ephemeris data. This information depends on the type of solar system object you 're dealing with. \\ | For Solar system objects, you can find information like the object type, and the object identification (name). Please forgive SkyChart when it shows you the Sun as a planet. All other information in this paragraph is dynamically calculated from the ephemeris data. This information depends on the type of solar system object you 're dealing with. \\ | ||
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| ==== Coordinates ==== | ==== Coordinates ==== | ||
| - | The coordinates of your object | + | The first line of this paragraph, starting with '' |
| + | The other lines show you the coordinates of your object in the specified coordinate systems. Here, you can find the equatorial systems (apparent and mean), and also in the ecliptic - and galactic systems. | ||
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| + | ==== Visibility for your observatory position and time ==== | ||
| + | Here you find specific data relating to your position and time. So there is the name of the site you are observing from with the **local date** and **time**. Next, you will find the times in **UT** and **local sideral time**. Then there is the positional data for the date and time that was used in the calculation: | ||
| - | ==== Visibility for observatory ==== | ||
| - | Here you find specific data relating to your position and time. So there is the name of the site you are observing from with the local date and time. Next, you will find the times in UT and local sideral time. Then there is the positional data for the date and time that was used in the calculation: | ||
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| Here you can find the distance and angle between two objects that you consecutively selected. This data can only reliably calculated when you select the objects from one single calculated chart or list. (A time difference combined with the dynamics of solar system objects can't lead to a precise value.) So, in order to retrieve distances, it can be wise to uncheck the **[[date_time# | Here you can find the distance and angle between two objects that you consecutively selected. This data can only reliably calculated when you select the objects from one single calculated chart or list. (A time difference combined with the dynamics of solar system objects can't lead to a precise value.) So, in order to retrieve distances, it can be wise to uncheck the **[[date_time# | ||
| First there is the line that says **which objects** you selected for the measurement. The next line shows the **seperation** in degrees of arc in sexagesimal format, and the **angle** measured from the previous to the last selected object. This angle takes the celestial North as zero reference, and increases by East, South, West. The picture is pretty self explanatory. About the angle: when you are on the Northern hemisphere and your face is directed south, the East will be at the left hand side. | First there is the line that says **which objects** you selected for the measurement. The next line shows the **seperation** in degrees of arc in sexagesimal format, and the **angle** measured from the previous to the last selected object. This angle takes the celestial North as zero reference, and increases by East, South, West. The picture is pretty self explanatory. About the angle: when you are on the Northern hemisphere and your face is directed south, the East will be at the left hand side. | ||
| - | The last line show you the **offset** in sexagesimal hours and sexagesimal degrees in the equatorial coordination system. | + | The last line shows you the **offset** in sexagesimal hours and sexagesimal degrees in the equatorial coordination system. |
en/documentation/detailed_information.1231716014.txt.gz · Last modified: 2015/11/06 20:34 (external edit)
