search
Get Started
search
IRAS - Space Mission
zoom_in Click to enlarge

IRAS

description IRAS Overview

The Infrared Astronomy Satellite (IRAS) operated from 1983 to 1989. This joint US, UK, and Dutch space mission conducted the first comprehensive all-sky survey using infrared light. Its data significantly advanced understanding of star formation, galaxy evolution, and the distribution of dust in our universe. Primarily used by astronomers and researchers studying celestial objects at infrared wavelengths.

help IRAS FAQ

What major discovery was the Infrared Astronomy Satellite (IRAS) known for?

Launched in 1983, IRAS is famous for conducting the first comprehensive all-sky survey at infrared wavelengths, leading to the discovery of infrared "cirrus" in the Milky Way. It also discovered the first dust disk around a star, Vega, hinting at potential planetary systems. Additionally, it identified several comets and asteroids, including the unusual object 3200 Phaethon.

Which space agencies collaborated to build and operate IRAS?

The IRAS mission was a joint international project involving NASA in the United States, the Netherlands Agency for Aerospace Programmes (NIVR), and the United Kingdom's Science and Engineering Research Council (SERC). The satellite was launched on a Delta rocket from Vandenberg Air Force Base. The mission operations and data processing were shared among the three partner nations.

How long did the IRAS mission last?

The IRAS satellite was launched in January 1983 and operated for 10 months until its liquid helium coolant was depleted in November 1983. The liquid helium was necessary to keep the infrared detectors cold enough to function and avoid thermal noise from the satellite itself. Although the official operational phase ended in 1983, the data it collected continued to be analyzed for years, with the catalog officially finalized in 1989.

Why did IRAS need to be cooled with liquid helium?

Infrared detectors are highly sensitive to heat, meaning that the satellite's own operating temperature would completely obscure the faint infrared light from distant stars and galaxies. To prevent this, the telescope was bathed in liquid helium to cool it down to just a few degrees above absolute zero. Once the coolant evaporated, the instrument became too warm to detect cosmic infrared radiation.

Reviews & Comments

Write a Review

rate_review

Be the first to review

Share your thoughts with the community and help others make better decisions.

Save to your list

Save your favorites and follow how their scores change over time.

Save favorites
Track changes
Compare scores

Already have an account? Sign in

Compare Items

See how they stack up against each other

Comparing
VS
Select 1 more item to compare