TIC 270584021
Eclipsing binaryNew candidate


Notes
| Type | Eclipsing binary |
| Status | New candidate |
| Period (days) | 3.9529284 |
| Period source | eclipse fit to TESS sectors [2, 29, 69, 96] |
| Eclipse / dip depth | 16.9% |
| Amplitude | 4.3% |
| RA (deg) | 347.707 |
| Dec (deg) | -34.3792 |
| TESS mag | 11.51 |
| TIC ID | 270584021 |
| SIMBAD name | not in SIMBAD |
| Nearest known variable | Gaia DR3 6555347938946736896 (YSO), 111" away |
| Data used | TESS sector 2 (QLP) |
| Found by | hunt.py (automatic) |
| Date | 2026-10-01 |
| Look it up | SIMBAD · VSX · ESASky · ExoFOP |
✦ Artist's impression
AI-painted · made locallyWhat this picture shows
Artist's impression of an UNCONFIRMED candidate, based on its measured data. Two stars of about 4,100 K and 3,800 K (0.8 and 0.4 times the Sun's radius, ~0.7 and ~0.6 solar masses) orbit each other every 94.9 hours, 7.9 million km apart (the Sun-Mercury distance is 58 million km). We see the orbit at 89 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. The painted look, surface detail and background were added by a locally run image AI; the stars' sizes, colours and spacing follow the measured data.
How it was made
Painted by an image AI (DreamShaper XL, a Stable Diffusion XL model) running locally on a home PC, over a 3D layout built from the measured data. No cloud services.
Data files
- 0_illustration.png 996 KB
- 4_eclipse_model.png 42 KB
- TIC270584021_s0002.fits 79 KB
- TIC270584021_s0002.png 40 KB
- model.json 772 B
- meta.json
