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#ASTRONOMY PLATE SOLVING SOFTWARE MANUAL#
#ASTRONOMY PLATE SOLVING SOFTWARE SOFTWARE#
#ASTRONOMY PLATE SOLVING SOFTWARE DOWNLOAD#
#ASTRONOMY PLATE SOLVING SOFTWARE WINDOWS#

#ASTRONOMY PLATE SOLVING SOFTWARE WINDOWS#

Most installer bundles for Windows deliver rather outdated versions.

Can mistake hot pixels for stars (a possible issue with DSLRs and other noisy sensors).

The downloading and installation of the correct and numerous index files is crucial for performance.

Reasonably fast when the mount's location is unknown or far off the expected position.

#ASTRONOMY PLATE SOLVING SOFTWARE DOWNLOAD#

It requires download of index files which can be installed through N.I.N.A., as well as the required index files that you need for your combination of focal length and pixel size. The local Astrometry.Net plate solver needs to be installed separately.

Blind Solver: Recommended when an Internet connection is available.

Does not need to know the camera's sensor pixel size or telescopes focal length.

Reliable when the mount's location is unknown or far off the expected position.

This requires the user to register for an account on Astrometry.Net and generate an API key that is then entered into the plate solve settings for Astrometry.Net. can upload the image to the API servers of Astrometry.Net for them to plate solve it.

Does not require an Internet connection.

Capable of fast blind solves even when the mount is far off the expected position.

It is downloaded and installed in two parts - the application itself, and its star database. URL: The ASTAP (Astrometric STAcking Program) astrometric solver and FITS file viewer is a powerful standalone plate solve application.

#ASTRONOMY PLATE SOLVING SOFTWARE SOFTWARE#

The following is a list of support plate solving software and their general characteristics. supports the most popular plate solving software suites available, each of which has its own benefits and drawbacks. and it is recommended that the application is set up to have a blind solver, should the preferred primary plate solver not work as expected. This is essential for a hands-off operation of N.I.N.A. Here plate solving will be triggered automatically and the parameters are used from the Plate Solving Options. Plate solving is also utilized in the Sequence to center on a given target and Automated Meridian Flip feature to recenter the scope after a flip occurred. This allows skipping the star alignment process that is typically done during a mount's start-up process.įor a precise centering with a given error margin use the "Repeat until error <" option. slew your mount to the location where it was supposed to be in the first place. The former will synchronize your mount's notion of its pointing position to the position that the plate solver has determined is it pointed. To apply the plate solving results to your mount, you need to enable the Sync option and, if desired, the Reslew To Target option in the Plate Solving panel. In the event that both the Primary and Blind plate solving applications fail to produce a result, please verify that your image is in focus and, if necessary, increase the exposure time or change the filter type to allow more stars to be adequately exposed. Thus, the Blind Solver acts as a back up method.īefore being able to plate solve N.I.N.A., any setup that the primary and blind solvers require must be done in accordance with their respective instructions. Where one fails to solve a given image, another might succeed. The reason for this is that while most plate solving software is quite good, none are infallible.

will prompt if the Blind Solver should be used to solve the image. There clicking on the play button a new image will be captured and solved based on the given parameters.

#ASTRONOMY PLATE SOLVING SOFTWARE MANUAL#

To manual trigger plate solve of an image you need to use the Plate Solving tool in the image panel. This includes the focal length of the telescope itself and any focal length-affecting devices such as reducers, telecompressors, or barlows.

will usually be able to detect the sensor's pixel size, but the user will need to inform the software of the effective focal length of the optical path. The two important settings are the camera's sensor pixel size and the focal length of the telescope. Plate solving requires that your camera and telescope settings are correct.