NASA SPHEREx · IPAC/IRSA DR1 · 0.75–5.0 µm
Module 01 · 6 min · Beginner

Infrared Vision

Why infrared astronomy matters

Try it: Galactic Centre, composite vs one channel
Real tile
3.29 / 1.91 / 0.85 µm
False-colour infrared composite
B1 0.75B2 1.11B3 1.66B4 2.44B5 3.83B6 4.434.99 µm
01

Seeing through dust

Interstellar dust scatters blue light far more than red. At 1–5 µm, starlight passes through clouds that are opaque in visible light, revealing young stars and the Galactic Centre.

02

Cool things glow in the infrared

Objects at a few hundred to a few thousand kelvin — brown dwarfs, dust, cool stars — emit most of their light at these wavelengths.

03

False colour, honestly labelled

Composites map three infrared channels to red, green and blue. They are not what the eye would see; the explorer always labels them as false-colour infrared.

Imagery & science data: NASA / Caltech-IPAC SPHEREx DR1 via IRSA. Catalogue overlay: d3-celestial (BSD-3).StellarScope · created by Vaishal Anil & Parthiv — Team The Abyss, NASA Space Apps 2026AI: IFM K2 Horizon · NVIDIA Nemotron · Spectral Scout v2 (ONNX)