NGC 4216

NGC 4216 is an edge-on spiral galaxy located not far from the center of the Virgo Cluster of galaxies. If the redshift of this galaxy was used to calculate the distance, it would be much smaller than expected. This is due to the internal motions of galaxies inside the Virgo Cluster. The entire group of galaxies is moving away from us, but NGC 4216 is moving towards us with respect to other group members. Thus, the net velocity for NGC 4216 is smaller than expected. Based on all information, this galaxy is roughly 40 million light years away. Inevitably astronomers will attempt to classify edge-on galaxies- which is often difficult due to the perspective we view them. In this case, many astronomers have measured aspects of this galaxy which lead them to believed it is a barred spiral galaxy, not unlike NGC 3953.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.

Créditos:

KPNO/NOIRLab/NSF/AURA/Ken Siarkiewicz/Adam Block

About the Image

Id:noao-n4216siarkiewicz
Tipo:Observation
Release date:2 de Abril de 2014 a las 12:54
Size:1747 x 1178 px

Sobre el Objeto

Nombre:NGC 4216
Constellation:Virgo
Categoría:Galaxies

Formatos de Imágenes

Large JPEGLarge JPEG
305,0 KB
Screensize JPEGScreensize JPEG
71,5 KB

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Coordenadas

ObjectValue
Posición (AR):12 15 53.65
Posición (Dec):13° 10' 38.74"
Campo visual:12.40 x 8.39 arcminutes
Orientación:North is 100.9° left of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
Optical
B
438 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
G
475 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
R
625 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
Broad Band
555 nmVisitor Center 0.5-meter Telescope
Other CCD