V456 Cep

STARB9 blue-white star

ILLUSTRATION FROM MEASURED TEMPERATURE · 13 500 K · 86.3 L☉ · VARIABLE, MAG 7.19–7.25 · PERIOD 1.268 DAYS · PULSE COMPRESSED

[

OVERVIEW

] STAR

V456 Cep is a B9 blue-white star in the constellation Cepheus, 898.5 from Earth, shining at apparent magnitude 7.21 (). It is catalogued as HD 217062 and HIP 113316.

WHAT IT IS
Blue-white star
HOW FAR
898.5

The light arriving now left it that long ago.

HOW BRIGHT (V)

Binoculars reach it; the naked eye does not.

WHERE TO LOOK
Cepheus

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

[

THE MODEL

] CATALOGUED RADIUS
OUTSIDE THE SURVEYED VOLUME · DRAG TO ORBIT

CALCULATED · NOT AN OBSERVATION · CATALOGUED RADIUS · MEASURED TEMPERATURE · 13 500 K · 86.3 L☉ · VARIABLE, MAG 7.19–7.25 · PERIOD 1.268 DAYS

Drawn from the catalogued radius and from the same properties the picture at the top of this page uses, at the distance a flight to it would stop. Drag it, or use the arrow keys, to look from another direction. The stars behind are the 498,631 this catalogue holds real distances for, drawn from where the camera actually is — but every one of them is within 170 parsecs of the Sun and this object is much further out, so what is in the frame is that whole neighbourhood seen from outside it, piled into a knot around the Sun. The rest of the sky from here is not something this catalogue knows.

[

OBSERVING

] FROM WHERE YOU ARE

What it takes to see V456 Cep 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 V456 Cep is worth going out for.

[

THROUGH AN EYEPIECE

] 150 MM TELESCOPE · 25 MM EYEPIECE
NE
2.3′ ACROSS

Too faint for your eyes alone. Binoculars reach it. Its brightest companion sits 54.5″ away, which at 48× is cleanly split.

48×
1.08
1.25
13.0
· AC
54.5 · cleanly split
· AB
4.40 · cleanly split
APPARENT MAGNITUDE ()
7.21 · within reach

A is where the pair was the year it was measured — the ones above, between 2003 and 2015, and a pair in a real orbit has moved since. The brightest companion — AC — is 2.4 magnitudes down on the star itself, which this far out from it is a faint speck beside a bright star rather than a matched pair.

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
11.8
PROPER MOTION SINCE
0.39

Computed for 2026-08-27 00:00 UT. Two things separate it from the catalogued position above: V456 Cep has moved under its own proper motion, and the coordinate grid has turned 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.

[

VARIABILITY

] ALPHA-2 CANUM VENATICORUM MAGNETIC ROTATING VARIABLE
RANGE, AS SAMPLED
7.19 – 7.25
PERIOD
1.26759 days (30.4 h)

The period is published and the epoch is not. A period says how long the cycle takes; without an observed maximum or minimum to count from there is no way to say which part of it the star is in tonight.

The range is the spread the Hipparcos satellite measured, converted to the visual scale. It is approximate: the satellite sampled the star on a schedule of its own, and where a star spends little of its cycle at an extreme — the floor of an eclipse, most obviously — the sampling can miss it altogether. The classification and the period are the General Catalogue of Variable Stars’s. These elements as data.

[

DOUBLE STAR

] 2 PAIRS
COMPONENTSSEPARATIONPOSITION ANGLEMAGNITUDEMEASURED
AB4.4″269°15.22003
AC54.5″81°9.562015

Separation and position angle are as measured in the year given; a position angle is measured from north, through east. Washington Double Star Catalog 22569+5958.

[

CATALOG DATA

] 19 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.

Spectral type
Surface temperature
13 491
Luminosity
86.2979
Luminosity (bolometric)
304.534
Radius
3.259
Mass
3.899
Surface gravity (log g)
Variability
Alpha-2 Canum Venaticorum magnetic rotating variable
Variability type ()
ACV:
Variability period
1.26759

HOW BRIGHT IT IS

What the light adds up to, measured through one filter at a time. A magnitude is a brightness on a backwards scale — the smaller the number, the brighter the object.

Colour index (B−V)
Variable magnitude, brightest
Variable magnitude, faintest

WHERE IT IS AND HOW IT MOVES

Position, motion across the sky and the size it covers on it. These are measurements of the object as seen from here, so every one of them depends on where here is.

Proper motion (RA)
14.18
Proper motion (Dec)
3.26
Radial velocity
0

OTHER NAMES AND NUMBERS

The identifiers other catalogues file this object under, for anyone joining this data to theirs.

Variable-star designation
V456 Cep
Washington Double Star id
22569+5958

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
Gaia DR3 model fit (GSP-Phot, FLAME; RUWE ≤ 1.4) — low confidence: above 7,500 GSP-Phot's temperature and extinction are degenerate
[

ALSO KNOWN AS

] 3 DESIGNATIONS
  • HD HD 217062
  • HIP HIP 113316
  • Variable star V456 Cep
[

LOOK IT UP ELSEWHERE

] 3 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. V456 Cep [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/hd-217062
BIBTEX
@misc{spacecatalog_hd-217062,
  author       = {{SpaceCatalog}},
  title        = {{V456 Cep}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/hd-217062},
  note         = {Catalogue entry, data release DR1 (2026-08-21). Values from HYG Database v4.1.}
}

The values above were taken from HYG Database v4.1 — CC-BY-SA-4.0. Citing this page does not replace citing that catalogue, and its licence is share-alike: the terms reach whatever you build from these rows.

[

RELATED OBJECTS

] 8 LINKED