PGC 130608

GALAXYElliptical galaxy E

ILLUSTRATION FROM HUBBLE TYPE E · MAJOR AXIS 0.516′ · AXIS RATIO 0.49 · POSITION ANGLE 54°

[

OVERVIEW

] GALAXY

PGC 130608 is an elliptical galaxy E in the constellation Indus, 247.4 from Earth, shining at apparent magnitude 16.20 (). Other catalogues list it as WISExSCOS J210608.84-470905.5.

WHAT IT IS
Elliptical galaxy
HOW FAR
247.4

A luminosity distance, from its redshift — how faint it looks. The light itself left 228 million years ago.

HOW BIG ON THE SKY
31

Small enough that the full Moon would cover it several times over.

HOW BRIGHT (B)

Faint: it takes a large telescope.

WHERE TO LOOK
Indus

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

[

THE MODEL

] LIGHT ALONG THE RAY
OUTSIDE THE SURVEYED VOLUME · DRAG TO ORBIT

CALCULATED · NOT AN OBSERVATION · ANGULAR SIZE AT THE CATALOGUED DISTANCE · HUBBLE TYPE E · MAJOR AXIS 0.516′ · AXIS RATIO 0.49 · POSITION ANGLE 54° · NO SURFACE — DRAWN AS A VOLUME · AXIS RATIO READ AS ITS OWN SHAPE

A spheroid whose brightness falls off as the quarter power of the radius, which is the profile de Vaucouleurs measured for elliptical galaxies and the profile the bulge of every spiral has. The shape of it is the catalogued class; the flattening is the catalogued axis ratio read as the object's own shape rather than as a tilt, because this is not a disc and its ellipticity is not an inclination. Nothing measured the depth, so what is drawn is the roundest object that matches the ellipse the catalogue holds. The two colours are two populations: old stars in the bulge and the disc, young ones in the arms, both through the same blackbody table as the star pages. 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 from here that whole neighbourhood is a knot in one direction and the rest of the sky is empty. The view you land on looks the other way; turn back towards the Sun and the stars come with it. What the readout says is which of the two the frame is pointed at. The emptiness is not a missing backdrop — it is the edge of what this catalogue has measured.

[

OBSERVING

] FROM WHERE YOU ARE

What it takes to see PGC 130608 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 PGC 130608 is worth going out for.

[

THROUGH AN EYEPIECE

] 150 MM TELESCOPE · 25 MM EYEPIECE
NE
FIELD 1.08°

Fainter than the largest telescope modelled here reaches. PGC 130608 covers 31″ of sky against a of 1.08°, so at 48× it is a speck in a wide field.

48×
1.08
1.25
13.0
SIZE ON THE SKY
31
FILLS OF THE FIELD
1% of the width
APPARENT MAGNITUDE ()
16.20 · too faint for this

PGC 130608 is not a point of light, so the limit above is the wrong one to hold it against: the same brightness spread over 31″ of sky is harder than a star of it, and goes first. Catalogued sizes are measured to a photographic contour, and the part an eye sees is usually smaller.

FIND IT ON THE SKY MAP ↗
[

APPARENT PLACE

] EQUINOX J2026.8

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
19.8
PROPER MOTION SINCE
none published

Computed for 2026-10-12 00:00 UT. No proper motion is published for PGC 130608, 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. The catalogue it came from publishes no error for that position, so nothing here says how far this arithmetic can be trusted — the digits above are as precise as the place they were computed from, and no more. Aberration, parallax and refraction are left out. Aberration swings every position by up to twenty arcseconds over a year; parallax stays under an arcsecond for all but the nearest stars; refraction is nothing overhead and about half a degree at the horizon, where it answers to the air, not the sky. The same figure for any date.

[

CATALOG DATA

] 9 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.

Hubble type
Stellar mass
6.54×10⁸ ±3.7×10⁸

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.

Apparent magnitude ()

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.

Redshift (z)
Redshift (z, CMB frame)
Major axis
0.51624
Minor axis
0.253629
54

WHERE THESE FIGURES CAME FROM

Which catalogue, paper or model each of the fields above was read from, where the source named one.

Morphology from
SIMBAD (1996MNRAS.278.1025L, quality D)
[

ALSO KNOWN AS

] 2 DESIGNATIONS
  • PGC PGC 130608
  • WISExSCOS WISExSCOS J210608.84-470905.5
[

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. PGC 130608 [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/pgc-130608
BIBTEX
@misc{spacecatalog_pgc-130608,
  author       = {{SpaceCatalog}},
  title        = {{PGC 130608}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/pgc-130608},
  note         = {Catalogue entry, data release DR1 (2026-08-21). Values from GLADE+ (Galaxy List for the Advanced Detector Era).}
}

The values above were taken from GLADE+ (Galaxy List for the Advanced Detector Era) — VizieR terms; cite Dalya+ 2022 (2022MNRAS.514.1403D). Citing this page does not replace citing that catalogue.

That catalogue asks for this acknowledgement: Dálya et al. 2022, MNRAS 514, 1403 (2022MNRAS.514.1403D) — "Please cite this paper when using GLADE+ data" — via VizieR VII/291. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in 2000, A&AS 143, 23.

[

RELATED OBJECTS

] 8 LINKED