M90

M90 is one of the few large spiral galaxies in the Virgo Cluster. This galaxy seems similar to M64 in that the outer arms are very smooth and devoid of star formation. In fact, there are few bright pink HII regions which might indicate any star birth in this galaxy. At a distance of 60 million light years away it is not alone and apparently disturbing its neighbor IC 3583. Astronomers have measured the velocity of this galaxy and have found that it is actually moving towards us! M90 has enough velocity to escape from the gravitational bonds of the Virgo Cluster of galaxies.

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

Créditos:

KPNO/NOIRLab/NSF/AURA/Paul and Daniel Koblas/Adam Block

About the Image

Id:noao-m90koblas
Tipo:Observation
Release date:24 de Febrero de 2014 a las 13:40
Size:972 x 1441 px

Sobre el Objeto

Nombre:M90
Constellation:Virgo
Categoría:Galaxies

Formatos de Imágenes

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219,4 KB
Screensize JPEGScreensize JPEG
162,2 KB

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Coordenadas

ObjectValue
Posición (AR):12 36 52.97
Posición (Dec):13° 8' 46.15"
Campo visual:8.36 x 12.40 arcminutes
Orientación:North is 82.2° right 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