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
Fondos de Pantalla
Coordenadas
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
Banda | Longitud de Onda | Telescopio |
---|---|---|
Optical B | 438 nm | Visitor Center Roll off Roof Observatory Other CCD |
Optical G | 475 nm | Visitor Center Roll off Roof Observatory Other CCD |
Optical R | 625 nm | Visitor Center Roll off Roof Observatory Other CCD |
Optical Broad Band | 555 nm | Visitor Center Roll off Roof Observatory Other CCD |