Cluster Stellar NGC 1333 (Chandra, Spitzer, DSS, Mayall)

Cluster Stellar NGC 1333 (Chandra, Spitzer, DSS, Mayall)

El clúster estelar NGC 1333 es el hogar de una gran cantidad de enanos marrones. Los astrónomos utilizarán los poderosos instrumentos infrarrojos de Webb para aprender más sobre estos primos tenues con las brillantes estrellas recién nacidas del clúster. Esta imagen se realizó combinando datos de los telescopios espaciales Chandra y Spitzer y los observatorios terrestres.

Credits

Image

NASA, CXC, SSC, NOAO, DSS

About The Object
Object Name NGC 1333
Object Description stellar cluster, reflection nebula
Constellation Perseus
Distance 1,000 light-years (306.6 parsecs)
About The Data
Data Description This new composite image of stellar cluster NGC 1333 combines X-rays from NASA's Chandra X-ray Observatory (pink); infrared data from NASA's Spitzer Space Telescope (red); and optical data from the Digitized Sky Survey and the National Optical Astronomical Observatories' Mayall 4-meter telescope on Kitt Peak near Tucson, Arizona. The Chandra data reveal 95 young stars glowing in X-ray light, 41 of which had not been seen previously using Spitzer because they lacked infrared emission from a surrounding disk.  
Instrument CXC, SST>Infrared Array Camera (IRAC), DSS, and NOAO>Mayall 4-meter telescope
Exposure Dates 7-2-2015
About The Image
Color Info Pink: Chandra X-ray Observatory
Red: Spitzer Space Telescope
Optical: DSS and Mayall 4-meter
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  • Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.