Free online converter for converting files to FITS.
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| Data type | Image |
| MIME type | image/fits |
| Developer | IAU FITS Working Group (international standard; widely supported by NASA/GSFC FITS community resources) |
| Primary use cases | Astronomical images, spectra, time series, 3D/4D data cubes (with time/wavelength axes), catalogs and calibration tables, long-term scientific archiving |
FITS is an open standard file format for astronomical images and scientific data arrays with rich metadata headers.
| Data type | Image |
| MIME type | image/fits |
| Compression | Optional; commonly uncompressed, or compressed via established FITS conventions (e.g., tiled image compression) |
| Color depth | BITPIX valid values: 8/16/32/64-bit integers and -32/-64 IEEE floating point |
| Color space | Not defined by the format; typically grayscale scientific values (intensity), with color rendering handled by the viewer |
| Metadata | Rich keyword/value headers (mandatory + optional + convention keywords). Headers are self-describing and store observation, instrument, WCS/time, and processing metadata |
| Standard / Specification | The FITS Standard, Version 4.0 (IAU FITS Working Group; approved 22 July 2016; language-edited 13 August 2018) |
| Typical file size | Highly variable: from small headers to many GB for large mosaics and multi-dimensional cubes; size depends on dimensions, BITPIX, and compression |
| Year introduced | 1981 |
The FITS file format offers several advantages that make it suitable for common use cases.
The FITS file format has certain limitations that may affect its use in specific scenarios.
FITS images are widely supported and can be viewed on most devices and platforms.
Treat FITS as untrusted input. Standard keywords are not inherently risky, but locally-defined conventions/keywords may trigger actions (e.g., reading other files/URIs or interacting with instruments). Large files may also stress resources
Open standard