KMT-2020-BLG-0414L
ILLUSTRATION FROM SPECTRAL TYPE WD · 40 000 K
OVERVIEW
] STARKMT-2020-BLG-0414L is a WD Wolf-Rayet star in the constellation Sagittarius, 3979 from Earth.
- WHAT IT IS
- Wolf-Rayet star
- HOW FAR
- 3979
The light arriving now left it that long ago.
OBSERVING
] FROM WHERE YOU AREWhat it takes to see KMT-2020-BLG-0414L for yourself. Everything in this part of the page is worked out for a real horizon, a real night and the equipment you say you have.
Say where you are, and this line says when KMT-2020-BLG-0414L is worth going out for.
APPARENT PLACE
] EQUINOX J2026.7Where a telescope has to be pointed today, which is not quite where the catalogue records the object: the coordinate grid itself has turned since the year 2000 the catalogue is referred to.
- RIGHT ASCENSION
- DECLINATION
- GRID TURNED SINCE
- 22.4
- PROPER MOTION SINCE
- none published
Computed for 2026-09-05 00:00 UT. No proper motion is published for KMT-2020-BLG-0414L, so nothing here moves the object; what separates this from the catalogued position above is the coordinate grid turning under it — about fifty arcseconds a year of precession since 2000, and the small nodding of the Earth’s axis on top of that. Aberration and refraction are not included, and neither is parallax; each is under an arcminute, which is also about as well as the catalogued position is known. The same figure for any date.
LIFE OF THIS STAR
] STAGE 3 OF 5KMT-2020-BLG-0414L is a Wolf-Rayet star — a heavy star whose own wind has stripped its outer layers away, leaving the fusing interior bare; within about three hundred thousand years it will collapse and explode as a supernova, leaving a black hole.
- COLLAPSING CLOUDtook about twenty thousand years
- MAIN SEQUENCElasted about three million years
- SUPERGIANTabout three hundred thousand years of itNOW
- SUPERNOVAbright for weeks, over in a second
- BLACK HOLEfor the rest of time
NOW The same swelling, on a star heavy enough to keep going: helium, then carbon, then a run of heavier elements each burning faster than the last, until the core is iron and fusion can release nothing more.
NEXT The iron core collapses in about a second and the rest of the star is thrown off at a tenth of the speed of light. For a few weeks it outshines the galaxy it is in.
EVERY STAGE ON THIS TRACK
- COLLAPSING CLOUDtook about twenty thousand years
- A cold clump of gas and dust falls in on itself and heats as it falls. It stops being a cloud and starts being a star at the moment its core is hot enough to fuse hydrogen.
- MAIN SEQUENCElasted about three million years
- Hydrogen fuses to helium in the core, and the outward push of that exactly balances the star's own weight. This is the long, steady stretch — nine-tenths of a star's life — and it ends when the core's hydrogen is gone.
- SUPERGIANTabout three hundred thousand years of itNOW
- The same swelling, on a star heavy enough to keep going: helium, then carbon, then a run of heavier elements each burning faster than the last, until the core is iron and fusion can release nothing more.
- SUPERNOVAbright for weeks, over in a second
- The iron core collapses in about a second and the rest of the star is thrown off at a tenth of the speed of light. For a few weeks it outshines the galaxy it is in.
- BLACK HOLEfor the rest of time
- Nothing the core could be made of is stiff enough to stop the collapse, so it does not stop. What remains is a region of space that light cannot leave.
- HOW FIRM Its hydrogen envelope has already been driven off by its own wind, which is a late and short-lived condition and one that only the heaviest stars reach.
Which stage KMT-2020-BLG-0414L is in was read from its catalogued class, its temperature and its total output at every wavelength — not from its brightness in visible light alone, which understates a cool star by a factor of several. The mass it started with is about thirty times the Sun's mass, from a published model fit, and that mass is what chooses the track. Every span of time here comes from the standard relation between a star’s mass and how long its fuel lasts, rounded to a single figure. They are orders of magnitude and none of them is a date.
CATALOG DATA
] 5 FIELDSThe raw catalogue values, as the source published them, with the error bars where one was published — sorted by what each set of figures is about rather than by the order they happened to be stored in.
WHAT KIND OF THING IT IS
What the object is in itself, rather than how it happens to look from here.
- Spectral type
- Mass
- 0.49
THE ORBIT
The shape of the path, where the object sits on it, and the instant those figures were true of. An orbit is a fit to observations and drifts away from the real one either side of its epoch.
- Stars in system
- 1
- Planets in system
- 2
WHERE THESE FIGURES CAME FROM
Which catalogue, paper or model each of the fields above was read from, where the source named one.
- Stellar parameters from
- NASA Exoplanet Archive composite parameters
LOOK IT UP ELSEWHERE
] 1 SERVICEEach link carries the identifier printed beside it. Nothing on this page is a measurement of our own, so a number that disagrees with one of these is worth reporting — and a service that has never catalogued this object under this name will say so plainly.
- VizieR5″ around 271.9150 -28.4852
Every published table with a row at this position, searched by coordinates rather than by name.
CITE THIS PAGE
] DR1This page is live and its numbers move when an upstream refreshes, so the citation names the release the rows belong to rather than the day you read them. The release itself is frozen, republished as a bundle, and is what a data-availability statement should point at.
SpaceCatalog. KMT-2020-BLG-0414L [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/kmt-2020-blg-0414l
@misc{spacecatalog_kmt-2020-blg-0414l,
author = {{SpaceCatalog}},
title = {{KMT-2020-BLG-0414L}},
howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
year = {2026},
url = {https://spacecatalog.org/object/kmt-2020-blg-0414l},
note = {Catalogue entry, data release DR1 (2026-08-21). Values from NASA Exoplanet Archive (Planetary Systems Composite Parameters).}
}The values above were taken from NASA Exoplanet Archive (Planetary Systems Composite Parameters) — Public domain (NASA). Citing this page does not replace citing that catalogue.