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Format

Flexible Image Transport System

Summary

Name
Flexible Image Transport System
Identifiers
  • MIME: image/fits
  • PUID: x-fmt/383
Format type
Image (Raster)
Description
Flexible Image Transport System (FITS) is an open standard defining a digital file format useful for storage, transmission and processing of data: formatted as multi-dimensional arrays (for example a 2D image), or tables. FITS is the most commonly used digital file format in astronomy. The FITS standard was designed specifically for astronomical data, and includes provisions such as describing photometric and spatial calibration information, together with image origin metadata. The FITS format was first standardized in 1981; it has evolved gradually since then, and the most recent version (4.0) was standardized in 2016. FITS was designed with an eye towards long-term archival storage, and the maxim once FITS, always FITS represents the requirement that developments to the format must be backward compatible.
File extensions
fits
Source
Digital Preservation Department / The National Archives

Internal signatures

FITS

Note
Header (SIMPLE, BITPIX and NAXIS card images)

Byte sequences

Min Frag Length
Absolute from BOF
Offset
0
Max offset
None
Byte Sequence
53494D504C4520203D202020202020202020202020202020202020202054{50}42495450495820203D{19}(2038|2B38|3038|3136|3332|3634){50}4E415849532020203D
Endianness
None

Changelog

  • Updated in V120

    Release date
    25 February 2025

    Flexible Image Transport System: New description added as part of PRONOM Research Week 2024. Submitted by Brigham Young University.