Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a2404c7b3f9d5094

Jump to content

// Workers AI · dad joke modeWhat did NGC 575 say to NGC 574? You're a galaxy behind.

From Wikipedia, the free encyclopedia
NGC 575
SDSS image
Observation data (J2000 epoch)
ConstellationPisces
Right ascension01h 30m 46.6s[1]
Declination+21° 26 26[1]
Redshift0.010434 ± 0.000017
Heliocentric radial velocity3128 ± 5 km/s
Distance145 ± 10 kly (44.4 ± 3.1 kpc)h1
0.73
Apparent magnitude (V)12.9
Apparent magnitude (B)13.6
Characteristics
TypeSB(rs)c[1]
Apparent size (V)1.7 × 1.6 arcseconds[2]
Other designations
IC 1710,[1] MCG+03-04-051,[1] PGC 5634,[1] UGC 1081
References: [1][2]

NGC 575 is a barred spiral galaxy of Hubble type SB(rs)c in the constellation Pisces. It is approximately 145 million light years from the Milky Way and has a diameter of about 70,000 light years.

The object was discovered on October 17, 1876, by Édouard Stephan (listed as NGC 575) and on January 18, 1896, by Stéphane Javelle (listed as IC 1710).[3]

References

[edit]
  1. 1 2 3 4 5 6 7 NASA/IPAC EXTRAGALACTIC DATABASE
  2. 1 2 SEDS: IC 1710
  3. Seligman, Courtney. "NGC 575". Celestial atlas. Retrieved 2026-01-10.
[edit]
  • Wikimedia Commons logo Media related to NGC 575 at Wikimedia Commons
  • SIMBAD Astronomical Database
  • Deep Sky Catalog