VISUAL ARCHIVE / IMAGE STORY

S301 at the Edge of Strong Gravity

An artist's view of a measured stellar orbit and a black-hole spin that remains to be determined.

Imagined star S301 curving around the Milky Way central black hole
AI-GENERATED CONCEPT ART / THE LAST TRANSMISSION

Artist’s impression of S301 near Sagittarius A. The star’s extreme orbit may let astronomers measure the central black hole’s spin through its effect on stellar motion. AI-generated illustration; sizes and distances are illustrative.*

THE OBSERVATION

What we can actually see.

Interferometric observations constrain S301's short, eccentric orbit near Sagittarius A*. The published analysis finds a path that could be sensitive to the central black hole's spin with further observations and spectroscopy.

THE ILLUSTRATION

What the artwork imagines.

The radiant disk, star trail, apparent proximity, and visible distortion are an interpretation of a region hidden by dust and unresolved in this form. The artwork does not show a photographed event horizon or an already measured spin.

FROM THE ILLUSTRATED ARTICLE

The story that inspired it.

The article follows a star that may have survived the breakup of a binary pair and explains how repeated passages could make a subtle prediction of general relativity measurable.

Read The Star Our Black Hole Kept

CHECK THE RECORD

The image interprets the research below. Follow the original work for the measurements and limits behind the scene.

S301 discovery paper

OTHER IMAGE STORIES

Keep looking.

Entire archive

CHANGE SCALE / THE DARK HEART

Follow the question
toward Sagittarius A*.

Move around an illustrated black hole, send a signal along a calculated light path, follow a star on an S2-inspired orbit, and release a probe into an orbit, escape, or plunge. Compare the model with the research behind this page.

Explore the black hole

THE SIGNAL CONTINUES

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