EARTH, Laniakea Supercluster—Somewhere in the southern sky, a star has been quietly crossing our galaxy for billions of years. Labeled SDSS J0715-7334, the star formed in the Milky Way’s largest companion galaxy—the Large Magellanic Cloud—and at some point drifted into our cosmic neighborhood.

Welcome, friend.

It is, by at least one important measure, the most chemically pristine star ever observed: nearly pure hydrogen and helium, with just 0.005 percent of the heavy elements found in our Sun, according to findings published in Nature Astronomy in April 2026.

In astronomy, “chemically pristine” basically means almost untouched by previous generations of stars. Our Sun is rich in heavier elements (carbon, oxygen, iron, etc.) because it was born from gas that had already been cooked and re‑cooked inside earlier stars.

J0715-7334 is different. To put that in perspective: if you melted down the Sun, about 2 percent of it would be heavy elements. Do the same thought experiment with this star, and you’d get almost nothing.

What makes the discovery stranger (and, frankly, more charming) is who found it. Not a team of seasoned astrophysicists hunched over supercomputers, but ten University of Chicago undergraduates on a class field trip to Chile.

The students were enrolled in a course called “Field Course in Astrophysics,” taught by Professor Alex Ji, deputy project scientist for the Sloan Digital Sky Survey’s fifth phase (SDSS-V). After weeks of sifting through SDSS data and flagging 77 candidate stars, they headed to Carnegie Science’s Las Campanas Observatory for Spring Break.

On their very first night, March 21, 2025, the second star they pointed the Magellan telescope at turned out to be the one.

“We found it the first night, and it completely changed our plans for the course,” Ji said in an SDSS press release.

In practice, “finding” a star like this means pattern‑matching, not sightseeing. Before they ever set foot in Chile, the students combed through SDSS catalogs for stars that looked suspiciously metal‑poor, then used Magellan to take spectra—breaking the starlight into a barcode of colors that reveals which elements are present.

For J0715-7334, the spectrum was nearly blank where astronomers expected to see heavy‑element fingerprints. The original plan had been to spend about ten minutes per target. Instead, once they saw what they had, the students observed J0715-7334 for three hours the following night.

“I was looking at that camera the whole night to make sure it was working,” said Natalie Orrantia, one of the students, in the same release.

So why does the star’s chemistry matter? Astronomers group all elements heavier than hydrogen and helium under the catch‑all label “metals,” and those metals accumulate over time as successive generations of stars live, die, and explode. A star with almost none of those metals had to have formed before most of that enrichment ever happened, when the universe was still young and relatively simple. J0715-7334 is, in effect, a surviving member of one of the earliest stellar generations we can still study directly.

Ji dubbed it an “ancient immigrant,” a relic from the earliest epochs of star formation that somehow ended up in our galaxy.

The team combined their spectral observations with motion data from the European Space Agency’s Gaia mission to trace the star’s orbit backward through time, confirming it originated in the Large Magellanic Cloud. Its carbon content was so low it couldn’t even be detected, a formation signature observed only once before.

The universe, it turns out, still has a few time capsules left to open. Sometimes, apparently, it’s the newcomers who find them first.