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TIC 239052493

Eclipsing binaryProbably known

Rare & notable finds

Nothing rare: all 10 checks came back clear. What was checked →

Checked, nothing found (8)

Microlensing (rogue planet?) · Superflare · Exocomet-shaped dip · Eclipse timing (third body?) · Eccentric eclipsing binary · Pulsating star in an eclipsing binary · Extra dips outside the eclipses · Type of star

Checked 2026-10-11 18:10 on NVIDIA GeForce RTX 4070, using every TESS sector of this star. All results (.json)

TIC239052493_s0019.png

Notes

WARNING: same period as the known variable V0432 Aur 57" away; the signal is probably its light leaking in. Found automatically by hunt.py in TESS sector 19 (flagged in 1 sector(s)). Detection score 2461.8. Not in VSX, ASAS-SN or ZTF variable catalogues at the time of the search; not in Gaia DR3's variable lists. Unchecked by hand yet: verify the period, nearby stars and a wider catalogue search. Updates: 2026-10-11 Gaia hints at a hidden companion star (RUWE 1.6) 2026-10-11 Found by the automatic search in TESS sector 19
The signal
TypeEclipsing binary
StatusProbably known
Period (days)3.07948
Period sourcehunt.py on TESS QLP sector 19
Eclipse / dip depth74.5%
Amplitude21.1%
Data usedTESS sector 19 (QLP)
The star (Gaia & TESS)
Distance (pc)501 (~1,635 light years)
Temperature (Gaia)5,245 K
Size (Gaia)4.24 x the Sun
Mass (Gaia)1.74 x the Sun
Luminosity (Gaia)11.80 x the Sun
Colour, Gaia BP-RP1.24
RUWE (Gaia)1.60 - hints at a hidden companion star
Gaia G mag11.06
TESS mag10.37
Names & neighbours
TIC ID239052493
Gaia DR3 ID189291376380056576
SIMBAD nameTYC 2416-1167-1 [*]
Nearest known variableV0432 Aur (EA+DSCT:, P = 3.0817 d), 57" away (same period!)
RA (deg)84.3657
Dec (deg)37.0866
Look it up SIMBAD · VSX · ESASky · ExoFOP
Record
Found byhunt.py (automatic)
Date2026-10-11
Last update2026-10-11

Where it sits among the stars

ESA Gaia colour and true brightness. Grey: every Star Log candidate. Orange: this star.

0123051015giantsmain sequencewhite dwarfscolour BP-RP (bluer ← → redder)brightness M_G (brighter ↑)

How to read this diagram →