NGC 5584 (Webb NIRCam + Hubble WFC3)

 NGC 5584 (Webb NIRCam + Hubble WFC3)

Combined observations from NASA’s NIRCam (Near-Infrared Camera) and Hubble’s WFC3 (Wide Field Camera 3) show spiral galaxy NGC 5584, which resides 72 million light-years away from Earth. Among NGC 5584’s glowing stars are pulsating stars called Cepheid variables and Type Ia supernova, a special class of exploding stars. Astronomers use Cepheid variables and Type Ia supernovae as reliable distance markers to measure the universe’s expansion rate.

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Credits

Image

NASA, ESA, CSA, Adam G. Riess (JHU, STScI)

Image Processing

Alyssa Pagan (STScI)

About The Object
Object Name NGC 5584
Object Description Spiral galaxy, cepheids host galaxy
R.A. Position 14:22:23.76
Dec. Position 00:23:15.61
Constellation Virgo
Distance About 72 million light-years (22 million parsecs)
About The Data
Data Description This image was created with Webb and Hubble data from proposals: and (A. Riess)
Instrument Hubble>WFC3/UVIS Webb>NIRCam
Exposure Dates 2 February 2023, Janurary-April 2011
Filters Hubble> F555W, F814W Webb> F277W
About The Image
Color Info This image is a composite of separate exposures acquired by the Hubble Space Telescope using the WFC3 instrument and the James Webb Space Telescope using the NIRCam instrument. Several filters were used to sample 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: F555W, Green: F814W, Red: F277W
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.