Globular Star Cluster NGC 1466

 Globular Star Cluster NGC 1466

This image from NASA's Hubble Space Telescope reveals an ancient, glimmering ball of stars called NGC 1466. It is a globular cluster — a gathering of stars all held together by gravity — that is slowly moving through space on the outskirts of the Large Magellanic Cloud, one of our closest galactic neighbors.

Blue straggler stars are blue, bright stars, with a higher mass than the average for a cluster, and they are expected to sink towards the center of a star cluster over time. Those closest to the cluster core are the first to migrate inwards, with more distant blue stragglers progressively moving inwards over time.

Credits

ESA and NASA

About The Object
Object Name NGC 1466
Object Description Globular Star Cluster
R.A. Position 03:44:32.99
Dec. Position 71:40:15.92
Constellation Hydrus
Distance The star cluster is located 160,000 light-years away from Earth.
Dimensions Image is about 2.66 arcmin across (about 124 light-years)
About The Data
Data Description The HST observations include those from program (A. Sarajedini).
Instrument HST>WFC3/UVIS; HST>ACS/WFC
Exposure Dates February and July 2016
Filters WFC3/UVIS: F336W and ACS/WFC: F606W, and F814W
About The Image
Color Info These images are a composite of separate exposures acquired by the WFC3/UVIS and the ACS/WFC instruments on the Hubble Space Telescope. Several filters were used to sample narrow and wide wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F336W Green = F606W Red = F814W
Compass Image Globular Star Cluster NGC 1466
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.