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SN 2005gj

Index SN 2005gj

SN 2005gj was a supernova located approximately 864 million light years (265 million parsecs) away from Earth. [1]

22 relations: Epoch (astronomy), Hydrogen, Hydrogen spectral series, Hypergiant, Light curve, Light-year, Luminous blue variable, Nearby Supernova Factory, Nebula, Neutron, Parsec, Princeton University Press, Quark, Quark-nova, Redshift, Sloan Digital Sky Survey, SN 2003fg, Spectral line, Supernova, Type Ia supernova, University of Calgary, White dwarf.

Epoch (astronomy)

In astronomy, an epoch is a moment in time used as a reference point for some time-varying astronomical quantity, such as the celestial coordinates or elliptical orbital elements of a celestial body, because these are subject to perturbations and vary with time.

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Hydrogen

Hydrogen is a chemical element with symbol H and atomic number 1.

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Hydrogen spectral series

The emission spectrum of atomic hydrogen is divided into a number of spectral series, with wavelengths given by the Rydberg formula.

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Hypergiant

A hypergiant (luminosity class 0 or Ia+) is among the very rare kinds of stars that typically show tremendous luminosities and very high rates of mass loss by stellar winds.

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Light curve

In astronomy, a light curve is a graph of light intensity of a celestial object or region, as a function of time.

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Light-year

The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.

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Luminous blue variable

Luminous blue variables (LBVs) are massive evolved stars that show unpredictable and sometimes dramatic variations in both their spectra and brightness.

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Nearby Supernova Factory

The Nearby Supernova Factory (SNfactory) is a collaborative experiment led by Greg Aldering, designed to collect data on more Type Ia supernovae than have ever been studied in a single project before, and by studying them, to increase understanding of the expanding universe and "Dark Energy." The project began as an outgrowth of the Supernova Cosmology Project at Lawrence Berkeley National Laboratory, but while the SCP focused on supernovae with redshifts of approximately 1.2, corresponding to a distance of 8.7 billion light years, SNfactory searches for nearby supernovae with redshifts of 0.03 to 0.08, corresponding to a distance of only 400 million to 1.1 billion light years.

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Nebula

A nebula (Latin for "cloud" or "fog"; pl. nebulae, nebulæ, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases.

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Neutron

| magnetic_moment.

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Parsec

The parsec (symbol: pc) is a unit of length used to measure large distances to astronomical objects outside the Solar System.

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Princeton University Press

Princeton University Press is an independent publisher with close connections to Princeton University.

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Quark

A quark is a type of elementary particle and a fundamental constituent of matter.

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Quark-nova

A quark-nova is the hypothetical violent explosion resulting from the conversion of a neutron star to a quark star.

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Redshift

In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum.

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Sloan Digital Sky Survey

The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States.

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SN 2003fg

SN 2003fg, sometimes called the "Champagne Supernova", was an unusual Type Ia supernova.

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Spectral line

A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies.

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Supernova

A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.

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Type Ia supernova

A type Ia supernova (read "type one-a") is a type of supernova that occurs in binary systems (two stars orbiting one another) in which one of the stars is a white dwarf.

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University of Calgary

The University of Calgary (U of C or UCalgary) is a public research university located in Calgary, Alberta, Canada.

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White dwarf

A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.

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Redirects here:

SN 2005 gj, SN2005 gj, SN2005gj.

References

[1] https://en.wikipedia.org/wiki/SN_2005gj

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