Star Vetter

TIC 229832383

An uncatalogued eclipsing-binary candidate from TESS.

CleanSurvivorP = 6.12677 d

Eclipsing-binary candidate: 6.1268-day period, a 3.02% primary eclipse, no significant secondary eclipse.

Primary eclipsetotal light 0.967
Surface brightness ratio
companion faint - no secondary eclipse
Companion temperature
below ~5,087 K
Companion / star radius
~0.17
Face hidden at primary eclipse
~3%
Separation
~9.4 x the star's radius
Eccentricity
consistent with circular

Zoomed: both stars drawn about 2x larger than their real size relative to the orbit, so they overlap for longer than the real eclipse lasts. A star's surface never gets dimmer during an eclipse - part of it is simply hidden. What drops is the total light we receive, shown exactly by the readout and bar below from the real light curve; the glow dims with it, exaggerated so small dips show. Colours follow temperature on a stellar colour scale, saturated so the differences show; the star's is its catalogue value (5,780 K). The companion's colour, sizes and orbit shape are estimates from the eclipse depths, duration and timing, assuming central eclipses and spherical stars - good to perhaps tens of percent. Only the relative orbit is shown; both stars really circle their common centre of mass. Animated about 22,056x faster than real on average, slowing down through each eclipse, and starting from where the system is in its orbit right now. Hover to pause.

  • Secondary2026-10-20 07:59 UTC
  • Primary2026-10-23 09:30 UTC
  • Secondary2026-10-26 11:01 UTC

Computed from the fitted ephemeris. Approximate - not corrected for your location or for light-travel time across Earth's orbit.

I

The signal

A repeating, consistent dip in brightness.

observed binned median residuals
-160000000000000-140000000000000-120000000000000-100000000000000-80000000000000-60000000000000-40000000000000-2000000000000000-0.4-0.20.00.20.4phase (P = 6.1268 d)relative flux

Residual scatter 1525048210437224.750% (observed minus binned median).

Clear, repeating eclipses with a consistent period and depth.

Period
6.12677 d
Primary depth
3.02%
Epoch (T0)
1628.862 BTJD
Duration
5.86 h
II

The catalog check

Cross-matched against known variable-star catalogs to rule out anything already listed.

  • VSXMatched
  • ASAS-SNNot found
  • Gaia eclipsing-binary tableNot found
  • Gaia variable classificationNot found
  • TESS EB catalog (Prsa+2022)Not found
  • ExoFOP TOI listNot found

1/6 catalogs list a known variable at this position.

!

A catalog lists a known variable at this position.

Catalogs checked
6
Matches
1
III

The pixel check

Confirms the dimming is on the target star, not a nearby source.

Out of eclipse
In eclipse
Difference (out - in)
+ target TIC 229832383x neighbour bright enough to cause the dipo other TIC starsO dimming centroid1 pixel = 21"

Out/in share one sqrt colour scale; in-eclipse = out-of-eclipse minus difference. TESS sector 12.

25.9
0.09 px2"
0.0050 phase
TIC 2298334230.54 px, dT 2.8
1.00
12

The dimming is centred on the target star. No nearby contaminant detected.

Centroid offset
0.09 px
Difference SNR
25.9
Capable neighbour
TIC 229833423
TESS sector
12
IV

The Gaia view

A second spacecraft's measurements: how far away the star is, how bright and what colour, and whether its position fits a single star.

The latest Gaia context file does not include this candidate yet, so there is no Gaia view to show.

V

The ground-survey check

An independent instrument, different years: does real ZTF photometry show the eclipse at the period TESS measured?

The latest ground-survey file does not include this candidate yet, so there is no independent ZTF check to show.

VI

Fold it yourself

Adjust the period and watch the eclipse appear.

-160000000000000-140000000000000-120000000000000-100000000000000-80000000000000-60000000000000-40000000000000-200000000000000-0.4-0.20.00.20.4phaserelative flux
6.12677

Shown at the true period. The raw light curve needed to re-fold at other periods has not been exported yet - this slider unlocks automatically once it is.

The period the pipeline measured. Drag the slider away from it and the eclipse smears out.

True period
6.12677 d
BLS period
6.12677 d
Odd/even z
0.03
VII

Caveats

Known limitations and things to check.

None found

No caveats flagged: this candidate cleared every gate with no named exception. Follow-up observations would still be needed to confirm the stellar parameters.

VIII

Instrument

Raw values, fits and technical details.

Show raw data

Full statistics

6.12677 d
6.12677 dsame
3.02% +/- 0.25%seen 2/3
< 1.93%none at 5 sigma
0.03< 3
13.9271 dpower 0.02
5.9 h
Distance (TIC, Gaia-based)
1029 pc+/- 37
14.05 / 13.31
5780 K / 2.46 Rsun
RA / Dec (J2000)
16h 36m 25.0s -44d 17m 52s
97.6 / 25.9
1,054 ptsover 28 d

Eclipse close-ups

Primary eclipse3.02%
-200000000000000-150000000000000-100000000000000-500000000000000-10010hours from mid-eclipse
Secondary (phase 0.500)not sig.
-200000000000000-150000000000000-100000000000000-500000000000000-10010hours from mid-eclipse

Same flux scale on both panels. Line: binned median. Shown in place of an orbit animation - this pipeline measures eclipses, it does not fit an orbit.

Period alias analysis

BLS period 6.1268 d
-150000000000000-100000000000000-500000000000000-0.50.00.5
2x BLS 12.2535 d
-200000000000000-150000000000000-100000000000000-500000000000000-0.50.00.5

Odd/even depth z = 0.03 (gate 3.0): alternate eclipses match, so the BLS period stands.

O - C timing

primary eclipses
only 2 fully-covered eclipse(s) in the data - at least 3 are needed to test the period for timing changes

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