TIC 156892633
Transit candidateRare, already known
Rare & notable finds
Something genuinely unusual turned up. Treat it as a lead: every one of these has ordinary explanations too, listed with each. How these checks work →
Already known: in SIMBAD as BD+43 1665 (*); catalogued variable star nearby: Gaia DR3 949833288821137536 (E, P = 2.4689 d), 265" away. The rare-find check confirms what is on record - still nice, but not a new discovery.
- Transit timing (TTV) significant
The transits arrive early or late by 2.9 min (typical error 1.1 min) repeating every ~57.3 orbits: something is tugging on the planet - another planet, or a moon.
Checked, nothing found (7)
Microlensing (rogue planet?) · Exocomet-shaped dip · Habitable zone & size · Transit duration (TDV) · Changing transit depth · Lopsided transit · Type of star
Checked 2026-10-11 16:22 on NVIDIA GeForce RTX 4070, using every TESS sector of this star. All results (.json)



Notes
The signal
| Type | Transit candidate |
| Status | Rare, already known |
| Period (days) | 0.8881684 |
| Period source | eclipse fit to TESS sectors [20, 47, 60] |
| Eclipse / dip depth | 1.6% |
| Amplitude | 1.7% |
| Data used | TESS sector 20 (QLP) |
Planet check
| Verdict | Probably noise or an instrument effect |
| Size if it's a planet | ~45.0 Earth radii (~4.01 Jupiter) - too big for a planet |
The star (Gaia & TESS)
| Distance (pc) | 292 (~952 light years) |
| Temperature (Gaia) | 6,238 K |
| Size (Gaia) | 3.05 x the Sun |
| Mass (Gaia) | 1.69 x the Sun |
| Luminosity (Gaia) | 12.73 x the Sun |
| Colour, Gaia BP-RP | 0.65 |
| RUWE (Gaia) | 1.60 - hints at a hidden companion star |
| Gaia G mag | 9.23 |
| TESS mag | 8.87 |
Names & neighbours
| TIC ID | 156892633 |
| Gaia DR3 ID | 949830097661078400 |
| SIMBAD name | BD+43 1665 [*] |
| Nearest known variable | Gaia DR3 949833288821137536 (E, P = 2.4689 d), 265" away |
| RA (deg) | 108.963 |
| Dec (deg) | 43.1264 |
| Look it up | SIMBAD · VSX · ESASky · ExoFOP |
Record
| Found by | hunt.py (automatic) |
| Date | 2026-10-11 |
| Last update | 2026-10-11 |
✦ Artist's impression
3D render · not AI-generated · made locallyWhat this picture shows
Artist's impression of an UNCONFIRMED candidate, based on its measured data. Two stars of about 6,200 K and 3,100 K (2.1 and 1.3 times the Sun's radius, ~1.2 and ~0.6 solar masses) orbit each other every 21.3 hours, 3.3 million km apart (the Sun-Mercury distance is 58 million km). We see the orbit at 50 degrees (90 = exactly edge-on), close enough to edge-on that they eclipse each other. Sizes, separation, tilt and colours come from fitting the TESS eclipses (see the model-fit plot) plus Gaia's temperature; masses assume normal main-sequence stars. Surface texture, glowing halos, the viewpoint and the background are artistic. The secondary eclipse arrives 64 minutes earlier than half an orbit after the primary, a sign of a slightly oval (eccentric) orbit: e*cos(omega) = -0.0785.
How it was made
A 3D render made in Blender on a home PC, not by AI.
Where it sits among the stars
ESA Gaia colour and true brightness. Grey: every Star Log candidate. Orange: this star.
Data files
- 0_illustration.png 2 MB
- 10_rare_check.png 26 KB
- 4_eclipse_model.png 54 KB
- 5_planet_check.png 127 KB
- TIC156892633_s0020.fits 76 KB
- TIC156892633_s0020.png 43 KB
- lightcurve_all_sectors.csv 551 KB
- model.json 769 B
- planet_check.json 4 KB
- rare_check.json 4 KB
- thumb.png 36 KB
- meta.json
