Hubble Ultra Deep Field

Creation and observational details

The HUDF observations were carried out over several months, with many individual exposures combined to build the final image. The original HUDF campaign took place between September 24, 2003 and January 16, 2004, requiring hundreds of exposures spread across many orbits of the Hubble telescope. The imaging used multiple instruments and filters to sample visible and near-infrared wavelengths, enabling astronomers to detect galaxies at a wide range of distances. The project exemplified the technique of very deep, narrow-field imaging to study the early universe and the most distant objects.

What the image contains

The HUDF reveals roughly ten thousand galaxies in a field that is extraordinarily small on the sky. To give a sense of scale, the patch covers only a few dozen square arcminutes—about one thirteen-millionth of the entire celestial sphere—and would appear smaller than a single grain of sand if viewed at arm's length. Many of the faint sources are compact early galaxies seen as they were billions of years ago; a subset appear as very red objects detectable primarily at infrared wavelengths, which indicate high redshift and therefore great distance and age. Observations combining Hubble's visible imaging with near-infrared data extended the reach of the HUDF to show galaxies whose light has been stretched by cosmic expansion into the infrared.

Key facts and coordinates

• Field location: southern celestial hemisphere near the constellation Fornax and southwest of Orion (Orion).
• Celestial co-ordinates (J2000): right ascension approximately 3h 32m 40s, declination approximately −27° 47′ 29″.
• Angular size: only a few dozen square arcminutes, a tiny fraction of the sky; the image orientation and reference stars have been cataloged for precise follow-up measurements.
• Exposure: hundreds of individual frames taken over many Hubble orbits; the long cumulative exposure time was essential to detect the faintest galaxies with Hubble.

Scientific importance

The HUDF has been instrumental in studies of galaxy formation and evolution. By providing a deep census of galaxy types, sizes, and colours across cosmic time, the image allows astronomers to investigate how the first galaxies assembled, how their star-formation rates changed, and how early structures contributed to cosmic reionization. Follow-up programs used the HUDF as a reference field for spectroscopy, gravitational lensing searches, and comparisons with ground-based infrared surveys counting galaxies and with other deep fields that sample different regions of the sky.

Distinguishing features and legacy

What sets the HUDF apart is the combination of extreme depth and high angular resolution in visible light. While large ground-based telescopes can detect faint infrared light, Hubble's stable platform above Earth's atmosphere allowed detailed visible-wavelength imaging of very faint, compact sources. The HUDF therefore complements other deep surveys and has inspired deeper and wider follow-up programs across multiple observatories. It remains a key reference for cosmological studies and a striking demonstration of how observing strategy—long exposures on a small area—can reveal the distant universe from Hubble and inform the design of future deep surveys with space telescopes and ground facilities working in the infrared.

1. For technical resources and datasets related to the HUDF, consult mission archives and instrument pages (RA/Dec details).
2. For summaries and scientific papers that interpret HUDF findings, see reviews and catalogues tied to the field (galaxy counts).
3. To compare the HUDF with other deep observations and outreach materials, explore curated image galleries and survey comparisons (survey context), (coordinate references), (positional data).

Researchers continue to build on the HUDF legacy by combining its dataset with newer observations at different wavelengths and resolutions. The image remains a powerful touchstone in observational cosmology, both for its scientific returns and for public appreciation of the distant universe.