TIC 431033666

Gaia DR3 2004767798943260288, 6 arcsec from BD+53 2845

Position: 22h 19m 04.51s, +53° 48′ 36.7″
V magnitude: 11.10
Where: 52 arcmin south of V345 Lac
Signal: EA, flat-bottomed primary, 68 days. The blended TESS light falls to about half. The bright B8 neighbor, TIC 431033672, falls about 19 percent at the same times. TESS does not say which star is eclipsed.

What TESS shows

Three flat-bottomed eclipses, in sectors 16, 56, and 84, fit

T0 = 1752.337 BTJD, P = 68.12269 d

The middle is the center of the run where the flux stays below 60 percent of normal. Measuring that center at 55, 60, or 80 percent moves the clock by about 10 minutes, so the prediction is good to about 20 minutes. The blended light stays 2 percent below normal for about 10.4 hours, and below 60 percent for about 3.8 hours. Half-period and one-third-period aliases do not eclipse. A shallow dip in sector 57 is not on this period.

The star is 6 arcseconds from BD+53 2845 (TIC 431033672, V = 9.84, spectral type B8, Gaia DR3 2004767798946201600). That brighter star’s extraction drops about 19 percent at the same three times, and the centroid does not move. A total eclipse of the fainter star, with the B8 star still in the aperture, fits the depth. TESS does not assign the eclipse. No other survey has a light curve that lands on these eclipses. The note is saved as a VSX draft, and that draft says the eclipse is not assigned to one star. No new observations are in it.

On 27 October 2026 the fade starts near 06:42 UTC, the deep part runs about 10:00 to 13:48 UTC, and the middle is 11:54 UTC. That start is still up from the western United States. The flat bottom is low in California and on the horizon in West Texas, in morning twilight. Recovery is after the star has set there. A measurement needs separate apertures on the two stars, a third comparison star, and a scale near one arcsecond per pixel.

The light curves

Six TESS sectors. The lines mark the 68-day ephemeris.

The faint star and the bright neighbor on the three eclipses.

The three eclipses folded on the 68.12-day period.

Finder chart

Real sky images (DSS2 red) with Gaia DR3 stars overlaid. North is up, east is left, J2000. Red tick marks point at the target (Gaia DR3 2004767798943260288, G = 11.04). Gold squares C1 to C5 are comparison stars of similar brightness. Tap an image for the full-size printable chart.

Wide finder, 30 × 30 arcmin, for star-hopping.

Close finder, 8 × 8 arcmin, to pick out the target.

	Gaia DR3	RA, Dec (J2000)	G	BP	RP	From target
C1	2004765325042124800	22:19:35.9 +53:47:33.9	10.17	10.32	9.89	4.8′
C2	2004763538335535360	22:19:05.5 +53:42:56.4	11.67	11.93	11.25	5.7′
C3	2004768692296667392	22:19:45.2 +53:49:21.1	11.34	11.63	10.88	6.1′
C4	2004763499666476288	22:19:12.1 +53:42:39.0	11.98	12.14	11.68	6.1′
C5	2004766046596429952	22:18:50.9 +53:42:22.7	11.98	12.36	11.44	6.5′

Comparison stars are within about 1 mag of the target in Gaia G, have similar color, no close companion, and no VSX entry within 10 arcsec. Images: DSS2 red (POSS-II, STScI Digitized Sky Survey). Stars: ESA Gaia DR3.

VSX

A VSX draft was saved on 15 October 2026. It says TESS does not assign the eclipse between this star and BD+53 2845. The draft is not in the public index. It waits while TIC 330739083 is the one star in review.

Next two eclipses

Eclipse 13 Jan 2027, 14:54 UTC · 3 Jan, 06:54 PST Pacific · 3 Jan, 15:54 CET central Europe
Eclipse 212 Mar 2027, 17:55 UTC · 12 Mar, 09:55 PST Pacific · 12 Mar, 18:55 CET central Europe

For each of those middles, the light is about 2 percent down from 5.2 hours before until 5.2 hours after, and below 60 percent of the blended light from 1.9 hours before until 1.9 hours after. The 27 October window in the paragraph above is that shape. The January eclipse has the same shape on the UTC clock.

Help with a measurement

The useful measurement is resolved photometry of the 6-arcsecond pair, so we learn which star fades. If that is you, pick a date below.

The note

A 68-day eclipse in the TESS aperture of TIC 431033666 (PDF)

These pages use the public TESS Quick-Look Pipeline and catalog positions. A prediction is not a confirmation. If you observe, write down which star was in the aperture.