NASA SPHEREx · IPAC/IRSA DR1 · 0.75–5.0 µm
Module 06 · 6 min · Beginner

Brown Dwarfs

What makes them interesting

Compare: a cool supergiant (Betelgeuse) — note the flags
DR1 cube
Extracting spectrum from the science cube… 0.0s

Bright stars saturate SPHEREx detectors; orange points carry FLAGS. A genuine brown dwarf would be faint, with deep 1.4/1.9 µm water bands.

01

Failed stars

Too light to sustain hydrogen fusion, brown dwarfs cool for ever. Their spectra show deep water and methane absorption.

02

What to look for

A spectrum rising toward 1–2 µm with dips near 1.4 and 1.9 µm is suggestive — but dust reddening can mimic slope, so evidence must be combined.

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)