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APOD: 2026 September 16 – Webb’s View of M64

APOD Science APOD APOD: 2026 September 16 –… Today’s APOD Archive Submissions Index Search Calendar RSS Education About Discuss   APOD Astronomy Picture of the Day Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. Hubble + WebbHubble […]

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APOD: 2026 September 16 –…

Today’s APOD

Archive

Submissions

Index

Search

Calendar

RSS

Education

About

Discuss

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

Hubble + WebbHubble

Webb’s View of M64

Explanation: Sometimes where Hubble finds darkness, Webb sees light. An example is today’s composite images of Messier 64 (M64), a nearby spiral galaxy of many names. The dark band of dust partially blocking its bright core earned it the moniker “the Black Eye Galaxy.” Webb’s Mid-InfraRed Instrument (MIRI) sees that dust, shown in red, as it absorbs and re-emits light from surrounding newborn stars. These young stars are embedded in pink star-forming regions in the Hubble-only image. M64’s inner and outer gas regions counter-rotate, creating regions of increased star formation where the two gas “currents” meet and compress. A merger between M64 and a smaller galaxy was likely the cause of the opposing motion of the outer gas. Spiral galaxies were once thought to have peaceful histories. M64 was key evidence that spiral galaxies, including the Milky Way, can and do experience mergers. Webb’s view of M64 will tell astronomers about the structure, motion, and composition of the galaxy’s dust and add context to the galaxy’s merger history and evolution.

APOD’s main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod

Tomorrow’s picture: treasure

Date:

September 16, 2026

Credit:

NASA, CSA, ESA, F. Belfiore (ESO), J. Lee (STScI), A. Leroy (OSU), and D. Thilker (JHU); Processing: G. Kober (NASA/Catholic University)

Authors & editors:

Keighley Rockcliffe, Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti

A service of:

ASD at NASA / GSFC,

NASA Science Activation & Michigan Tech. U.

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