M88

M88 displays a set of tight spiral arms and dust lanes in each. A recent supernova (1991) in M88 helped better determine its distance from us. Stars exploding in other galaxies can be used as a "standard candle" since astronomers know their intrinsic brightness (how bright it would appear at a known distance). Then, by measuring the brightness of the supernova, they can estimate its distance by using the properties of light (things appear dimmer the further away they are). M88 is calculated to be 60 million light years away by this method.

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

Créditos:

KPNO/NOIRLab/NSF/AURA/Jim Quinn/Adam Block

About the Image

Id:noao-m88quinn
Tipo:Observation
Release date:20 de Febrero de 2014 a las 13:48
Size:2184 x 1472 px

Sobre el Objeto

Nombre:M88
Constellation:Coma Berenices
Categoría:Galaxies

Formatos de Imágenes

Large JPEGLarge JPEG
428,6 KB
Screensize JPEGScreensize JPEG
96,9 KB

Zoomable


Fondos de Pantalla

1024x7681024x768
124,0 KB
1280x10241280x1024
202,7 KB
1600x12001600x1200
286,8 KB
1920x12001920x1200
338,0 KB
2048x15362048x1536
1,9 MB

Coordenadas

ObjectValue
Posición (AR):12 32 1.37
Posición (Dec):14° 23' 25.58"
Campo visual:12.42 x 8.32 arcminutes
Orientación:North is 179.2° 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