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: a2385ce2cef70acb

Jump to content

// Workers AI · dad joke modeWhat did NGC 442 say to NGC 441? You're a star neighbor.

From Wikipedia, the free encyclopedia

NGC 442
NGC 442
SDSS view of NGC 442
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 14m 38.6s[1]
Declination−01° 01 14[1]
Redshift0.018640[1]
Heliocentric radial velocity5,588 km/s[1]
Distance261.58 Mly (80.200 Mpc)[1]
Apparent magnitude (V)14.45[1]
Absolute magnitude (V)-22.42[1]
Characteristics
TypeS0/a? (edge on)[1]
Apparent size (V)1.0' × 0.5'[1]
Other designations
UGC 00789, CGCG 385–041, MCG +00-04-054, 2MASX J01143863-0101139, 2MASXi J0114385-010113, 6dF J0114385-010114, 6dFGSv 00692, PGC 4484.[1]

NGC 442 is a spiral galaxy of type S0/a? (edge on) located in the constellation Cetus. Lewis Swift discovered it on October 21, 1886. Dreyer first described it as "very faint, small, round, bright star to southeast." The star is actually located northeast of NGC 442, but, due to the way optical telescopes worked, it was not unusual for some confusion of directions to occur.[2]

References

[edit]
  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 0442. Retrieved September 2, 2016.
  2. "New General Catalog Objects: NGC 400 - 449". Cseligman. Retrieved April 22, 2017.
[edit]
  • Wikimedia Commons logo Media related to NGC 442 at Wikimedia Commons