It's a Bird, It's a Plane, No It's Mira!

Galex_glx2007-04r_img02_1024

galex_glx2007-04r_img02 August 15th, 2007

Credit: NASA/JPL-Caltech/C. Martin (Caltech)/M. Seibert(OCIW)

A close-up view of a star racing through space faster than a speeding bullet can be seen in this image from NASA's Galaxy Evolution Explorer. The star, called Mira (pronounced My-rah), is traveling at 130 kilometers per second, or 291,000 miles per hour. As it hurls along, it sheds material that will be recycled into new stars, planets and possibly even life.

In this image, Mira is moving from left to right. It is visible as the pinkish dot in the bulb shape at right. The yellow dot below is a foreground star. Mira is traveling so fast that it's creating a bow shock, or build-up of gas, in front of it, as can be seen here at right.

Like a boat traveling through water, a bow shock forms ahead of the star in the direction of its motion. Gas in the bow shock is heated and then mixes with the cool hydrogen gas in the wind that is blowing off Mira. This heated hydrogen gas then flows around behind the star, forming a wake.

Why is the wake of material glowing? When the hydrogen gas is heated, it transitions into a higher-energy state, which then loses energy by emitting ultraviolet light Ð a process called fluorescence. The Galaxy Evolution Explorer has special instruments that can detect this ultraviolet light.

A similar fluorescence process is responsible for the Northern Lights -- a glowing, green aurora that can be seen from northern latitudes. However, in that case nitrogen and oxygen gas are fluorescing with visible light.

Streams and a loop of material can also be seen coming off Mira. Astronomers are still investigating what these streams are, but they suspect that they are denser parts of Mira's wind perhaps flowing out of the star's poles.

This image consists of data captured by both the far- and near-ultraviolet detectors on the Galaxy Evolution Explorer between November 18 and December 15, 2006. It has a total exposure time of about 3 hours.

Provider: Galaxy Evolution Explorer

Image Source: /image/galex/glx2007-04r_img02

Curator: Galaxy Evolution Explorer

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Image Details Image Details

Image Type
Observation
Object Name
Mira
Subject - Milky Way
Star > Evolutionary Stage > Red Giant

Distance Details Distance

Universescale1
300 light years

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
GALEX (FUV) Ultraviolet (Far-UV) 150.0 nm
GALEX (NUV) Ultraviolet (Near-UV) 230.0 nm
Spectrum_base
Galex_glx2007-04r_img02_1280
×
ID
glx2007-04r_img02
Subject Category
B.3.1.4.  
Subject Name
Mira
Credits
NASA/JPL-Caltech/C. Martin (Caltech)/M. Seibert(OCIW)
Release Date
2007-08-15
Lightyears
300
Redshift
300
Reference Url
/image/galex/glx2007-04r_img02
Type
Observation
Image Quality
Good
Distance Notes
Facility
GALEX, GALEX
Instrument
FUV, NUV
Color Assignment
Band
Ultraviolet, Ultraviolet
Bandpass
Far-UV, Near-UV
Central Wavelength
150, 230
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
Equinox
Reference Value
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
FITS Header
Notes
Creator (Curator)
Galaxy Evolution Explorer
URL
http://www.galex.caltech.edu
Name
Email
Telephone
Address
City
State/Province
Postal Code
Country
Rights
Publisher
Galaxy Evolution Explorer
Publisher ID
galex
Resource ID
Resource URL
/image/galex/glx2007-04r_img02
Related Resources
Metadata Date
2023-04-12T00:38:57Z
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
300 light years

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