V2376 Ori b

EXOPLANETGas giant

ILLUSTRATION FROM EQUILIBRIUM TEMPERATURE 2100 K · RADIUS 7.78 JUPITER RADII · HOST STAR M

[

OVERVIEW

] EXOPLANET

V2376 Ori b is a in the constellation Orion. It orbits V2376 Ori at a mean distance of 71 . It has a mass of 20.00 and a radius of 7.78 · 556 208 . It was discovered in 2025.

WHAT IT IS
Gas giant
HOW FAR
71

Its average distance from V2376 Ori, not from Earth.

HOW BIG
7.78 · 556 208

Its radius: half the width across.

WHERE TO LOOK
Orion

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

[

OBSERVING

] FROM WHERE YOU ARE

What it takes to see V2376 Ori b 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 V2376 Ori b is worth going out for.

[

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
19.7
PROPER MOTION SINCE
none published

Computed for 2026-08-27 00:00 UT. No proper motion is published for V2376 Ori b, 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.

[

CATALOG DATA

] 8 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 IT IS MADE OF

What the object is in itself, rather than how it happens to look from here.

Equilibrium temperature
2100
Host star spectral type
Host star mass
0.45 ±0.05

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.

Host star
V2376 Ori
Stars in system
1
Planets in system
1

WHEN IT WAS FOUND

Who first saw it, from where, and by what method.

Discovery method
Imaging
Discovered at
Multiple Observatories
[

ALSO KNOWN AS

] 2 DESIGNATIONS
  • Exoplanet V2376 Ori b
  • Host star V2376 Ori
[

LOOK IT UP ELSEWHERE

] 4 SERVICES

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. V2376 Ori b [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/v2376-ori-b
BIBTEX
@misc{spacecatalog_v2376-ori-b,
  author       = {{SpaceCatalog}},
  title        = {{V2376 Ori b}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/v2376-ori-b},
  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