| NGC 3776 | |
|---|---|
 Image of NGC 3776 from the Sloan Digital Sky Survey | |
| Observation data (J2000epoch) | |
| Constellation | Virgo |
| Right ascension | 11h 38m 17.98s |
| Declination | -03° 21′ 15.8″ |
| Redshift | 0.03784 |
| Heliocentric radial velocity | 11,130 km/s |
| Apparent magnitude (V) | 16.0 |
| Surface brightness | 23.0 mag/arcsec2 |
| Characteristics | |
| Type | Sb |
| Apparent size (V) | 0.48′ × 0.38′ |
| Notable features | Part of the New General Catalogue (NGC) of deep-sky objects |
| Other designations | |
| [Add any additional catalog names or designations] | |
NGC 3776 is aspiral galaxy located in theconstellation Virgo. It is classified as anSb-type galaxy, which signifies it has moderately tightly woundspiral arms. This galaxy was discovered in 1886 by astronomerOrmond Stone, known for his work cataloging celestial objects in thesouthern hemisphere. NGC 3776 has avisual magnitude of 16, making it challenging to observe without a telescope. The galaxy is cataloged within theNew General Catalogue (NGC), a comprehensive listing of deep-sky objects compiled byJohn Louis Emil Dreyer in 1888 to include discoveries like Stone’s.
NGC 3776 is anSb-type spiral galaxy, characterized by its moderately tight spiral arms. Located in the constellation Virgo, this galaxy is observable at right ascension 11h 38m 17.98s and declination -03° 21′ 15.8″.[1][2] The galaxy has an apparentvisual magnitude of 16.0, making it relatively faint and challenging to view without advanced telescopic equipment. Itsradial velocity of approximately 11,130 km/s andredshift of 0.03784 indicate a substantialrecessional velocity, which is consistent with galaxies positioned at considerable distances fromEarth.[3]
NGC 3776 has a surface brightness of about 23.0 mag/arcsec2, which suggests that it appears dim against the night sky. With an angular size of 0.48′ by 0.38′, it occupies a small region when viewed from Earth. These measurements highlight its remoteness and modestluminosity compared to more prominent galaxies.
NGC 3776 was discovered in 1886 by the American astronomerOrmond Stone, who made significant contributions to the study of southern hemisphere celestial objects during his tenure at theLeander McCormick Observatory inVirginia.
