Difference between revisions of "Gustav Kirchhoff" - New World Encyclopedia

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'''Gustav Robert Kirchhoff''' (March 12, 1824 – October 17, 1887) was a [[Germany|German]] [[physicist]] who contributed to the fundamental understanding of [[electrical circuit]]s, [[spectroscopy]], and the emission of [[black-body]] radiation by heated objects. He coined the term "black body" radiation in 1862, and two sets of independent concepts in both circuit theory and thermal emission are named "[[Kirchhoff's laws]]" after him.
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'''Gustav Robert Kirchhoff''' (March 12, 1824 – October 17, 1887) was a [[Germany|German]] [[physicist]] who contributed to the fundamental understanding of [[electrical circuit]]s, [[spectroscopy]], and the emission of [[black-body]] radiation by heated objects. He coined the term "black body" radiation in 1862, and two sets of independent concepts in both circuit theory and thermal emission are named "[[Kirchhoff's laws]]" after him.
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== Biography ==
 +
 
 +
=== Early life ===
  
 
Gustav Kirchhoff was born in [[Kaliningrad|Königsberg]], [[East Prussia]], the son of  Friedrich Kirchhoff, a lawyer, and Johanna Henriette Wittke.  He graduated from the Albertus University of Königsberg in 1847 where he attended the mathematico-physical seminar directed by [[Franz Ernst Neumann]] and Friedrich Julius Richelot.  He married Clara Richelot, the daughter of his mathematics professor Richelot.  In the same year, they moved to [[Berlin]], where he stayed until he received a professorship at [[Wrocław|Breslau]].
 
Gustav Kirchhoff was born in [[Kaliningrad|Königsberg]], [[East Prussia]], the son of  Friedrich Kirchhoff, a lawyer, and Johanna Henriette Wittke.  He graduated from the Albertus University of Königsberg in 1847 where he attended the mathematico-physical seminar directed by [[Franz Ernst Neumann]] and Friedrich Julius Richelot.  He married Clara Richelot, the daughter of his mathematics professor Richelot.  In the same year, they moved to [[Berlin]], where he stayed until he received a professorship at [[Wrocław|Breslau]].
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 +
=== Scientific work ===
  
 
Kirchhoff formulated his [[Kirchhoff's circuit laws|circuit laws]], which are now ubiquitous in [[electrical engineering]], in 1845, while still a student.  He completed this study as a seminar exercise; it later became his doctoral dissertation.  He proposed his [[Kirchhoff's law of thermal radiation|law of thermal radiation]] in 1859, and gave a proof in 1861. He was called to the University of [[Heidelberg]] in 1854, where he collaborated in spectroscopic work with [[Robert Bunsen]]. Together Kirchhoff and Bunsen discovered [[caesium]] and [[rubidium]] in 1861 while studying the chemical composition of the [[Sun]] via its spectral signature.  At Heidelberg he ran a mathematico-physical seminar, modelled on Neumann's, with the mathematician Leo Koenigsberger.  Among those who attended this seminar were [[Arthur Schuster]] and [[Sofia Kovalevskaya]]. In 1875 Kirchhoff accepted the first chair specifically dedicated to theoretical physics at [[Berlin]].
 
Kirchhoff formulated his [[Kirchhoff's circuit laws|circuit laws]], which are now ubiquitous in [[electrical engineering]], in 1845, while still a student.  He completed this study as a seminar exercise; it later became his doctoral dissertation.  He proposed his [[Kirchhoff's law of thermal radiation|law of thermal radiation]] in 1859, and gave a proof in 1861. He was called to the University of [[Heidelberg]] in 1854, where he collaborated in spectroscopic work with [[Robert Bunsen]]. Together Kirchhoff and Bunsen discovered [[caesium]] and [[rubidium]] in 1861 while studying the chemical composition of the [[Sun]] via its spectral signature.  At Heidelberg he ran a mathematico-physical seminar, modelled on Neumann's, with the mathematician Leo Koenigsberger.  Among those who attended this seminar were [[Arthur Schuster]] and [[Sofia Kovalevskaya]]. In 1875 Kirchhoff accepted the first chair specifically dedicated to theoretical physics at [[Berlin]].
  
 
In 1862 he was awarded the [[Rumford Medal]] for his researches on the fixed lines of the solar spectrum, and on the inversion of the bright lines in the spectra of artificial light.
 
In 1862 he was awarded the [[Rumford Medal]] for his researches on the fixed lines of the solar spectrum, and on the inversion of the bright lines in the spectra of artificial light.
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=== Death ===
  
 
Kirchhoff died in 1887, and was buried in the St Matthäus Kirchhof Cemetery in [[Schöneberg]], [[Berlin]], only a few meters from the graves of the [[Brothers Grimm]].
 
Kirchhoff died in 1887, and was buried in the St Matthäus Kirchhof Cemetery in [[Schöneberg]], [[Berlin]], only a few meters from the graves of the [[Brothers Grimm]].
  
== Spectroscopy research ==
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== Details of scientific work ==
 
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=== Circuit Laws ===
He contributed greatly to the field of spectroscopy by formalizing three laws that describe the [[optical spectrum|spectral]] composition of [[light]] emitted by incandescent objects, building substantially on the discoveries of [[David Alter]] and [[Anders Jonas Angstrom]] (see also: [[spectrum analysis]])
 
 
 
''Kirchhoff's Three Laws of Spectroscopy:''
 
 
 
#A hot solid object produces light with a continuous spectrum.
 
#A hot tenuous gas produces light with [[spectral line]]s at discrete [[wavelength]]s (i.e. specific colors) which depend on the energy levels of the atoms in the gas.  (''See also:'' [[emission spectrum]])
 
#A hot solid object surrounded by a cool tenuous gas (i.e. cooler than the hot object) produces light with an almost continuous spectrum which has gaps at discrete wavelengths depending on the energy levels of the atoms in the gas. (''See also:'' [[absorption spectrum]])
 
 
 
The existence of these discrete lines was later explained by the [[Bohr model]], which helped lead to the development of [[quantum mechanics]].
 
 
 
== Circuit Laws ==
 
 
[[Image:KCL.png|framed|The current entering any junction is equal to the current leaving that junction. ''i''<sub>1</sub> + ''i''<sub>4</sub> = ''i''<sub>2</sub> + ''i''<sub>3</sub>]]
 
[[Image:KCL.png|framed|The current entering any junction is equal to the current leaving that junction. ''i''<sub>1</sub> + ''i''<sub>4</sub> = ''i''<sub>2</sub> + ''i''<sub>3</sub>]]
 
[[Image:KVL.png|framed|The sum of all the voltages around the loop is equal to zero. v<sub>1</sub> + v<sub>2</sub> + v<sub>3</sub> + v<sub>4</sub> = 0]]
 
[[Image:KVL.png|framed|The sum of all the voltages around the loop is equal to zero. v<sub>1</sub> + v<sub>2</sub> + v<sub>3</sub> + v<sub>4</sub> = 0]]
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'''Kirchhoff's circuit laws''' (or circuit rules) are a pair of laws that deal with the [[Charge conservation|conservation of charge]] and energy in [[electrical circuit]]s, and were first described in [[1845]] by [[Gustav Kirchhoff]]. Widely used in [[electrical engineering]], they are also called Kirchhoff's ''rules'' or simply Kirchhoff's ''laws''.
 
'''Kirchhoff's circuit laws''' (or circuit rules) are a pair of laws that deal with the [[Charge conservation|conservation of charge]] and energy in [[electrical circuit]]s, and were first described in [[1845]] by [[Gustav Kirchhoff]]. Widely used in [[electrical engineering]], they are also called Kirchhoff's ''rules'' or simply Kirchhoff's ''laws''.
  
=== Kirchhoff's Current Law (KCL)===
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==== Kirchhoff's Current Law (KCL)====
  
 
The current law is also called '''Kirchhoff's first law''', '''Kirchhoff's point rule''', '''Kirchhoff's junction rule''', and '''Kirchhoff's first rule'''. It is based on the principle of conservation of [[electric charge]], which implies that:
 
The current law is also called '''Kirchhoff's first law''', '''Kirchhoff's point rule''', '''Kirchhoff's junction rule''', and '''Kirchhoff's first rule'''. It is based on the principle of conservation of [[electric charge]], which implies that:
 
:At any point in an [[electrical circuit]] where [[charge density]] is not changing in time, the sum of [[current (electricity)|current]]s flowing toward that point is equal to the sum of currents flowing away from that point.
 
:At any point in an [[electrical circuit]] where [[charge density]] is not changing in time, the sum of [[current (electricity)|current]]s flowing toward that point is equal to the sum of currents flowing away from that point.
  
=== Kirchhoff's Voltage Law (KVL) ===
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==== Kirchhoff's Voltage Law (KVL) ====
  
 
The voltage law is also called '''Kirchhoff's second law''', '''Kirchhoff's loop rule''', and '''Kirchhoff's second rule'''. It is a consequence of the principle of [[conservation of energy]], which implies that:
 
The voltage law is also called '''Kirchhoff's second law''', '''Kirchhoff's loop rule''', and '''Kirchhoff's second rule'''. It is a consequence of the principle of [[conservation of energy]], which implies that:
 
:The directed sum of the electrical [[potential difference]]s around a circuit must be zero.
 
:The directed sum of the electrical [[potential difference]]s around a circuit must be zero.
 +
 +
=== Spectroscopy research ===
 +
 +
He contributed greatly to the field of spectroscopy by formalizing three laws that describe the [[optical spectrum|spectral]] composition of [[light]] emitted by incandescent objects, building substantially on the discoveries of [[David Alter]] and [[Anders Jonas Angstrom]] (see also: [[spectrum analysis]])
 +
 +
''Kirchhoff's Three Laws of Spectroscopy:''
 +
 +
#A hot solid object produces light with a continuous spectrum.
 +
#A hot tenuous gas produces light with [[spectral line]]s at discrete [[wavelength]]s (i.e. specific colors) which depend on the energy levels of the atoms in the gas.  (''See also:'' [[emission spectrum]])
 +
#A hot solid object surrounded by a cool tenuous gas (i.e. cooler than the hot object) produces light with an almost continuous spectrum which has gaps at discrete wavelengths depending on the energy levels of the atoms in the gas. (''See also:'' [[absorption spectrum]])
 +
 +
The existence of these discrete lines was later explained by the [[Bohr model]], which helped lead to the development of [[quantum mechanics]].
  
 
==See also==
 
==See also==
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[[Category:Biography]]
 
[[Category:Biography]]
  
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Revision as of 01:46, 28 March 2007


Gustav Robert Kirchhoff

Gustav R. Kirchhoff.jpg
Gustav Kirchhoff
Born

12 March, 1824
Königsberg, East Prussia

Died 17 October, 1887

Berlin, Germany

Residence Flag of Germany.svg Germany
Nationality Flag of Germany.svg German
Field Physicist
Institutions University of Berlin
University of Breslau
University of Heidelberg
Alma mater University of Königsberg
Academic advisor  Franz Ernst Neumann
Notable students  Max Noether
Ernst Schröder
Known for Kirchhoff's circuit laws
Kirchhoff's law of thermal radiation
Notable prizes Rumford medal

Gustav Robert Kirchhoff (March 12, 1824 – October 17, 1887) was a German physicist who contributed to the fundamental understanding of electrical circuits, spectroscopy, and the emission of black-body radiation by heated objects. He coined the term "black body" radiation in 1862, and two sets of independent concepts in both circuit theory and thermal emission are named "Kirchhoff's laws" after him.

Biography

Early life

Gustav Kirchhoff was born in Königsberg, East Prussia, the son of Friedrich Kirchhoff, a lawyer, and Johanna Henriette Wittke. He graduated from the Albertus University of Königsberg in 1847 where he attended the mathematico-physical seminar directed by Franz Ernst Neumann and Friedrich Julius Richelot. He married Clara Richelot, the daughter of his mathematics professor Richelot. In the same year, they moved to Berlin, where he stayed until he received a professorship at Breslau.

Scientific work

Kirchhoff formulated his circuit laws, which are now ubiquitous in electrical engineering, in 1845, while still a student. He completed this study as a seminar exercise; it later became his doctoral dissertation. He proposed his law of thermal radiation in 1859, and gave a proof in 1861. He was called to the University of Heidelberg in 1854, where he collaborated in spectroscopic work with Robert Bunsen. Together Kirchhoff and Bunsen discovered caesium and rubidium in 1861 while studying the chemical composition of the Sun via its spectral signature. At Heidelberg he ran a mathematico-physical seminar, modelled on Neumann's, with the mathematician Leo Koenigsberger. Among those who attended this seminar were Arthur Schuster and Sofia Kovalevskaya. In 1875 Kirchhoff accepted the first chair specifically dedicated to theoretical physics at Berlin.

In 1862 he was awarded the Rumford Medal for his researches on the fixed lines of the solar spectrum, and on the inversion of the bright lines in the spectra of artificial light.

Death

Kirchhoff died in 1887, and was buried in the St Matthäus Kirchhof Cemetery in Schöneberg, Berlin, only a few meters from the graves of the Brothers Grimm.

Details of scientific work

Circuit Laws

The current entering any junction is equal to the current leaving that junction. i1 + i4 = i2 + i3
The sum of all the voltages around the loop is equal to zero. v1 + v2 + v3 + v4 = 0

Kirchhoff's circuit laws (or circuit rules) are a pair of laws that deal with the conservation of charge and energy in electrical circuits, and were first described in 1845 by Gustav Kirchhoff. Widely used in electrical engineering, they are also called Kirchhoff's rules or simply Kirchhoff's laws.

Kirchhoff's Current Law (KCL)

The current law is also called Kirchhoff's first law, Kirchhoff's point rule, Kirchhoff's junction rule, and Kirchhoff's first rule. It is based on the principle of conservation of electric charge, which implies that:

At any point in an electrical circuit where charge density is not changing in time, the sum of currents flowing toward that point is equal to the sum of currents flowing away from that point.

Kirchhoff's Voltage Law (KVL)

The voltage law is also called Kirchhoff's second law, Kirchhoff's loop rule, and Kirchhoff's second rule. It is a consequence of the principle of conservation of energy, which implies that:

The directed sum of the electrical potential differences around a circuit must be zero.

Spectroscopy research

He contributed greatly to the field of spectroscopy by formalizing three laws that describe the spectral composition of light emitted by incandescent objects, building substantially on the discoveries of David Alter and Anders Jonas Angstrom (see also: spectrum analysis)

Kirchhoff's Three Laws of Spectroscopy:

  1. A hot solid object produces light with a continuous spectrum.
  2. A hot tenuous gas produces light with spectral lines at discrete wavelengths (i.e. specific colors) which depend on the energy levels of the atoms in the gas. (See also: emission spectrum)
  3. A hot solid object surrounded by a cool tenuous gas (i.e. cooler than the hot object) produces light with an almost continuous spectrum which has gaps at discrete wavelengths depending on the energy levels of the atoms in the gas. (See also: absorption spectrum)

The existence of these discrete lines was later explained by the Bohr model, which helped lead to the development of quantum mechanics.

See also

  • Kirchhoff equations
  • Spectroscopy
  • Spectrum analysis

References
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