NN Ser

STARWD Wolf-Rayet star

ILLUSTRATION FROM MEASURED TEMPERATURE · 40 000 K

[

OVERVIEW

] STAR

NN Ser is a WD Wolf-Rayet star in the constellation Serpens, 1682 from Earth, shining at apparent magnitude 16.94 ().

WHAT IT IS
Wolf-Rayet star
HOW FAR
1682

The light arriving now left it that long ago.

HOW BRIGHT (V)

Faint: it takes a large telescope.

WHERE TO LOOK
Serpens

The patch of sky it sits in, as seen from Earth.

[

OBSERVING

] FROM WHERE YOU ARE

What it takes to see NN Ser 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.

TONIGHT

Say where you are, and this line says when NN Ser is worth going out for.

[

THROUGH AN EYEPIECE

] 150 MM TELESCOPE · 25 MM EYEPIECE
EYE50MM150MM300MM16.94
TELESCOPE REACHES 13.0

Fainter than the largest telescope modelled here reaches. It will be a point of light in anything: a star is far enough away that no aperture on Earth gives it a width, and all the equipment changes is how easily you find it.

48×
1.08
1.25
13.0
APPARENT MAGNITUDE ()
16.94 · too faint for this
FIND IT ON THE SKY MAP ↗
[

APPARENT PLACE

] EQUINOX J2026.7

Where 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
19.1
PROPER MOTION SINCE
none published

Computed for 2026-08-28 00:00 UT. No proper motion is published for NN Ser, 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 5

NN Ser 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.

  1. COLLAPSING CLOUD
    took about twenty thousand years
  2. MAIN SEQUENCE
    lasted about three million years
  3. SUPERGIANT
    about three hundred thousand years of it
    NOW
  4. SUPERNOVA
    bright for weeks, over in a second
  5. BLACK HOLE
    for 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 NN Ser 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

] 6 FIELDS

The 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
Surface temperature
57 000
Mass
0.535

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
2
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 SERVICE

Each 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.

[

CITE THIS PAGE

] DR1

This 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.

PLAIN TEXT
SpaceCatalog. NN Ser [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/nn-ser
BIBTEX
@misc{spacecatalog_nn-ser,
  author       = {{SpaceCatalog}},
  title        = {{NN Ser}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/nn-ser},
  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.

[

RELATED OBJECTS

] 8 LINKED