What is different about the Cloverleaf is the huge quantity of dense gas along with very powerful
infrared radiation from the star formation.
Beta Pictoris entered the limelight over 20 years ago when NASA's Infrared Astronomical Satellite detected excess
infrared radiation from the star.
Not exact matches
Infrared radiation passes through interstellar dust much more easily than visible light, so by looking at the infrared light from a galaxy we can learn about the new stars forming within the clouds of dust
Infrared radiation passes through interstellar dust much more easily than visible light, so by looking at the
infrared light from a galaxy we can learn about the new stars forming within the clouds of dust
infrared light
from a galaxy we can learn about the new
stars forming within the clouds of dust and gas.
The lack of
infrared glow
from the galaxy across a broad range of wavelengths, however, suggests that there's very little dust there to absorb and then re-radiate the
stars»
radiation, the team notes.
By observing the combined
infrared radiation of
star and planet with Spitzer and then subtracting the
radiation recorded
from the
star alone when it hid the planet, Deming and Charbonneau had detected the heat of the planet itself.
In the past 2 decades, astronomers have detected
infrared radiation from debris disks around several
stars.
They combined observations in the visible and the near
infrared from the Hubble Space Telescope with radio observations
from the Very Large Array and the Submillimeter Array to explore the effect of the turbulence, stellar
radiation, and magnetic field on massive
star formation in the galaxy's nuclear ring.
Marois and his team used ground - based
infrared detection to seek out exoplanets around nearby, young, massive
stars — those whose planets would have wide orbits and emit significant amounts of
radiation as they cool
from their relatively recent births millions of years ago.
In 1983, an orbiting satellite called IRAS discovered far more
infrared radiation — which has waves longer than red light — coming
from the Vega than expected for small interstellar dust grains found around young, early - type
stars (Harvey et al, 1984).
Webb's giant sunshield will protect it
from stray heat and light, while its large mirror enables it to effectively capture
infrared light, bringing us the clearest picture ever of space objects that emit this invisible
radiation beyond the red end of the visible spectrum — early galaxies, infant
stars, clouds of gas and dust, and much more.
61 Virginis is a yellow - orange main sequence dwarf of spectral and luminosity type G5 - 6 V, with about 92 to 96 percent of Sol's mass (95 percent using the isochrone mass estimate of Valenti and Fischer, 2005; and NASA
Star and Exoplanet Database, based on David F. Gray, 1992), 94 to 98 percent of its diameter (96 percent for Valenti and Fischer, 2005; Johnson and Wright, 1983, page 677; and NASA
Star and Exoplanet Database, derived
from the exponential formula of Kenneth R. Lang, 1980), and around 78 percent of its visual luminosity and nearly 81 percent of its theoretical bolometric luminosity, with
infrared radiation (Sousa et al, 2008; Valenti and Fischer, 2005; NASA
Star and Exoplanet Database, based on Kenneth R. Lang, 1980).
A starburst galaxy has an exceptionally high rate of
star birth, first identified by its excess of
infrared radiation from warm dust.
The data also will be studied for evidence of a faint, uniform
infrared background, the residual
radiation from the first
stars and galaxies formed following the Big Bang.