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: a23ec55a1c8c0d7f

Jump to content

NGC 140

From Wikipedia, the free encyclopedia
NGC 140
NGC 140 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationAndromeda[1]
Right ascension00h 31m 20.5s[2]
Declination+30° 47 33[2]
Redshift0.021458[2]
Heliocentric radial velocity6433 km/s[2]
Apparent magnitude (V)13.94[2]
Characteristics
TypeScd[1]
Apparent size (V)1.35' × 1.15'[1]
Notable features"Very faint, small, round, gradually brighter middle."[1]
Other designations
UGC 311,[2] PGC 1916[1]

NGC 140 is a spiral galaxy in the constellation of Andromeda. It was discovered by Truman Henry Safford on October 8, 1866.[1]

Historical Information

[edit]

Safford's discovery in 1866 was published in the appendix of an obscure paper. Sixteen years later, on November 5, 1882, Edouard Stephan discovered the same object, but was unaware of Safford's earlier discovery. Wolfgang Steinicke's version of the catalog lists Safford as the discoverer.[1]

Supernova

[edit]

One supernova has been observed in NGC 140: SN 2025wug (Type IIb, mag. 16)[3] was discovered by ATLAS on 2 September 2025.

References

[edit]
  1. 1 2 3 4 5 6 7 Seligman, Courtney. "NGC Objects: NGC 100-149-NGC 140". Celestial Atlas. Retrieved 29 May 2016.
  2. 1 2 3 4 5 6 "NED results for the object NGC 0140". NASA/IPAC Extragalactic Database. Retrieved 29 May 2016.
  3. "SN 2025wug". Transient Name Server. IAU. Retrieved 8 September 2025.
[edit]
  • Wikimedia Commons logo Media related to NGC 140 at Wikimedia Commons