NGC 4490

This pair of galaxies often goes by the nickname of the "Cocoon Galaxy." Each "blob" is actually a spiral galaxy that has been distorted by the other. Hints of spiral structure are still evident in the smaller galaxy. These galaxies have already passed through their closest approach (perigalacticon) and are now speeding away from each other. A tail of stars stretches between the galaxies which are separated by at least 24,000 light years. All of this action takes place 40-50 million light years away. These interacting galaxies make a good real-world example for astronomers to compare computer models (simulations) of galactic collisions. Note the incredible number of starforming regions that have developed along facing sides of each galaxy.

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

Créditos:

KPNO/NOIRLab/NSF/AURA/Michael Gariepy/Adam Block

About the Image

Id:noao-n4490gariepy
Tipo:Observation
Release date:4 de Febrero de 2014 a las 12:39
Size:2184 x 1472 px

Sobre el Objeto

Nombre:NGC 4490
Constellation:Canes Venatici
Categoría:Galaxies

Formatos de Imágenes

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469,2 KB
Screensize JPEGScreensize JPEG
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Coordenadas

ObjectValue
Posición (AR):12 30 17.56
Posición (Dec):41° 37' 43.16"
Campo visual:12.38 x 8.36 arcminutes
Orientación:North is 101.6° right of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
Optical
B
438 nmVisitor Center Roll off Roof Observatory
Other CCD
Optical
G
475 nmVisitor Center Roll off Roof Observatory
Other CCD
Optical
R
625 nmVisitor Center Roll off Roof Observatory
Other CCD
Optical
Broad Band
555 nmVisitor Center Roll off Roof Observatory
Other CCD