science & techESA/Hubble

Dust dims distant supernovae; two wavelengths let astronomers separate dust from distance

the gist

Type Ia supernovae are the standard candles of astronomy: they come from white dwarfs and reach a very consistent peak brightness, so how dim they appear reveals how far away they are. The catch is that dust between us and the explosion also dims the light. Astronomers solve this by photographing the same supernova in ultraviolet light, which dust blocks heavily, and in infrared light, which passes through almost untouched. The difference between the two reveals how much dust is in the way, so the true brightness can be recovered. Hubble can observe both wavelengths with the same instrument, which makes it ideal for this calibration. NGC 3810, the galaxy here, hosted a Type Ia supernova in 2022 and sits about 50 million light-years away.

how it works

A white dwarf that gains mass from a companion can reach a critical limit and detonate with a predictable peak luminosity. Dust scatters and absorbs blue and ultraviolet light much more than red and infrared, so comparing colours shows how much light was lost to dust rather than distance.

so what

This method underpins measurements of how fast the universe is expanding, because distances to remote galaxies rest on the supernova yardstick, and dust is one of the biggest sources of error.

the bigger pattern

Astronomers use a cosmic distance ladder, where each rung is calibrated by the one below. Cepheid variable stars, whose brightness is linked to their pulsation period, let Edwin Hubble show in the 1920s that galaxies lie far beyond the Milky Way, and supernovae extend that ladder to the most distant galaxies.

fun fact

Type Ia supernovae were central to the 1998 discovery that the expansion of the universe is accelerating.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA, D. Sand, R. J. Foley