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Answer · HD 139139, the "Random Transiter"

The dips are astrophysical, on star A or star B.

The dips are astrophysical, on star A or star B.

Most likelyAnswers 1 questionPublished0

Where it stands

Most likelyIts test partly supported it: three pieces of evidence for, none against. It needs two reviews to be accepted.

What it predicts

  • The dips appear in independent reductions (K2SFF, EVEREST, Kepler pipeline).
  • The flux centroid does not move during dips.
  • Dips recur in later sensitive photometry of the pair.

What would rule it out

  • Later monitoring at sufficient precision, over several weeks, that finds no dips; or an identified detector or pointing effect that reproduces them.

Evidence 3 for · none against

Tested by 1 run

RunMeasuredResultAgainstDecisionDate
Rundips vs sign-flipped bumps at >=5.5 sigma; published dips recovered{'EVEREST': [19, 4], 'K2SFF_all': [23, 12], 'K2SFF_ge1.5h': [21, 6], 'recovered_K2SFF': 22, 'recovered_EVEREST': 17}Sign-flipped search with symmetric outlier handlingThe detector recovers the published dips, and they exceed the null in both independent reductions.

The questions it answers

Most likelyThe dips are astrophysical, on star A or star B

Cite it

Mysteries Department. (2026). The dips are astrophysical, on star A or star B. [Answer ANS0D79S0VG5ZJW]. https://mysteriesdept.com/r/ANS0D79S0VG5ZJW
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