¡Lo sentimos! Esta página aún no está disponible en su idioma preferido, por lo que estamos mostrando la versión original.
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
Fondos de Pantalla
Coordenadas
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
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 |