science & techESA/Hubble

Hubble is mapping cosmic dust around Type Ia supernovae to measure the universe more accurately

the gist

Type Ia supernovae are explosions of dead white dwarf stars, and they are useful because they have roughly the same intrinsic brightness. Astronomers compare how bright one looks from Earth with how bright it should be, which gives its distance and that of its host galaxy. This galaxy, about 600 million light-years away in Gemini, hosts SN 2022aajn, a supernova discovered in November 2022 and photographed here about two months after that. Dust between galaxies makes distant supernovae look fainter and redder, which can throw off distance estimates. To separate the two effects, Hubble will survey 100 Type Ia supernovae across seven wavelength bands, since infrared light passes through dust more easily than visible light. The result should sharpen measurements of how fast the universe is expanding.

how it works

A Type Ia supernova occurs when a white dwarf pulls in matter from a companion star until it reaches a critical mass and detonates, producing nearly the same peak brightness each time. Comparing observed and expected brightness gives distance. Dust scatters and absorbs blue light more than infrared, so comparing several wavelengths lets astronomers correct for it.

so what

Supernova distances were used to discover in 1998 that the expansion of the universe is accelerating, and dust is one of the largest sources of error in that work. Better dust correction tightens estimates of the expansion rate, one of the big open questions in cosmology.

fun fact

The 1998 discoveries of accelerating expansion came from teams studying Type Ia supernovae, and the work earned a Nobel Prize in Physics in 2011.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz)