RESOLVING THE LEDGER
RESOLVING THE LEDGER
Only one outlet has reported this event so far — you're reading it below, credited to its source. AIPROPX is tracking the web for more coverage; as additional outlets confirm it, this becomes a full multi-source story automatically.
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For decades, astronomers lumped brown dwarfs into a single category defined by mass alone—too big to be classified as planets but too small to become stars. However, this definition ignores the two very different mechanisms that can form them: the direct collapse of gas clouds and formation within the accretion disks of massive stars.
Indexed and credited by AIPROPX. Originating outlet: Phys.org. Open at source →
An original, deterministic readout — composed only from the computed coverage facts on this page. No interpretation, no rating; figures only.
AIPROPX has consolidated 1 report from 1 outlet into a single canonical entry on “TESS discovers a rare brown dwarf orbiting a massive, aging star.” Every covered outlet is based in Other.
The only timestamped report came from Phys.org (Aug 13, 2026, 21:00 UTC).
2 statements are carried by only one outlet within this set and are not echoed by the others.
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AIPROPX — “TESS discovers a rare brown dwarf orbiting a massive, aging star” · https://www.aipropx.com/story/0f0d4b1d05655a9ca8fcce0c0e91cc30
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