Draperjeva točka: Razlika med redakcijama

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[[Slika:Hot metalwork.jpg|250px|thumb|desno|Draperjevo točko se lahko ponazori kot temno rdeči prehod med svetlim in temnim delom kovinske palice.]]
'''Draperjeva točka''' je približna [[temperatura]], pri kateri skoraj vse [[trdnina|trdnine]] oddajajo [[vidna svetloba|vidno svetlobo]] zaradi [[sevanje črnega telesa|sevanja črnega telesa]]. Znaša 525 °C (798 K oz. 977 °F), določil pa jo je [[John William Draper]] leta [[1847 v znanosti|1847]].<ref>{{cite journal| journal = The Academy| title = Science: Draper's Memoirs| volume = XIV| issue = 338 | author = Murray, J. | date = 1878 | page = 408 | url = http://books.google.com/books?id=hZINAAAAQAAJ&pg=PA408&dq=draper+point+red+1847&lr=&as_brr=0&ei=6sxtSpnpLoLglATlh4RW}}</ref><ref>{{cite book| title = Radiation heat transfer: a statistical approach| author = Mahan, J.R. | edition = 3| publisher = Wiley-IEEE| year = 2002| isbn = 978-0-471-21270-6| page = 58| url = http://books.google.com/books?id=y9zUEzA7iN0C&pg=PA58&dq=draper-point+red&lr=&as_drrb_is=q&as_minm_is=0&as_miny_is=&as_maxm_is=0&as_maxy_is=&as_brr=3&ei=H8ttSo_2LImMkQTwvuxO}}</ref><ref>{{cite journal| title = Production of Light by Heat
| author = Draper, J.W. | journal = The London, Edinburgh and Dublin philosophical magazine and journal of science| year = 1847| page = 345&ndash;359| url = http://books.google.com/books?id=VEgEAAAAYAAJ&pg=PA345}}</ref>
 
'''Draperjeva točka''' je približna [[temperatura]], pri kateri skoraj vse [[trdnina|trdnine]] oddajajo [[vidna svetloba|vidno svetlobo]] zaradi [[sevanje črnega telesa|sevanja črnega telesa]]. Znaša 525 °C (798 K oziroma 977 °F), določil pa jo je [[John William Draper]] leta [[1847 v znanosti|1847]].<ref>{{sktxt|Murray|1878|pp=408}}.</ref><ref>{{sktxt|Mahan|2002|pp=58}}.</ref><ref>{{sktxt|Draper|1847}}.</ref>
Telesa pod to temperaturno točko sevajo v glavnem v [[infrardeče valovanje|infrardečem delu spektra]], torej pri daljših [[valovna dolžina|valovnih dolžinah]], in oddajajo zanemarljivo malo vidne svetlobe. Vrednost Draperjeve točke se lahko izračuna iz [[Wienov zakon|Wienovega zakona]]:<ref>{{cite book |title= Statistical Physics|last= Wannier|first= G.H.|year= 1987|origyear= 1966|publisher=Dover Publications|location= New York|isbn= 978-0-486-65401-0|oclc= 15520414|chapter= Chapter 10-2}}</ref>
 
Telesa pod to temperaturno točko sevajo v glavnem v [[infrardeče valovanje|infrardečem delu spektra]], torej pri daljših [[valovna dolžina|valovnih dolžinah]], in oddajajo zanemarljivo malo vidne svetlobe. Vrednost Draperjeve točke se lahko izračuna iz [[Wienov zakon|Wienovega zakona]]:<ref>{{cite book sktxt|title= Statistical Physics|last= Wannier|first= G.H.|year= 1987|origyear= 1966|publisher=Dover Publications|location= New York|isbn= 978-0-486-65401-0|oclc= 15520414|chapter= Chapter 10-2}}.</ref>
:<math>\nu_{vrh} = { 2.821 \over h} kT ,</math>
 
: <math> \nu_{\rm vrh} = \frac{ 2.,821}{h} k_{\overrm hB} kTT \!\, , </math>
kjer je
 
kjer je:
:*''k'' [[Boltzmannova konstanta]],
 
:*''k''<sub>B</sub> [[Boltzmannova konstanta]],
:*''h'' [[Planckova konstanta]],
:*''T'' temperatura (v kelvinih[[kelvin]]ih),
:*''ν''<sub>vrh</sub>'' frekvenca vrha sevanja pri Draperjevi točki.
 
Z izračunom dobimose dobi frekvenco vrha sevanja, ki znaša 46,9 terahercov (THz), kar se nahaja ravno na prehodu iz infrardečega spektra sevanja v slabo vidno temno rdečo barvo.<ref>{{cite book sktxt| title = Biology: Concepts and Applications | author = Starr, C. | publisher = Thomson Brooks/Cole | year = 2005 | isbn = 0-534-46226-X | url = http://books.google.com/books?id=RtSpGV_Pl_0C&pg=PA94}}.</ref>
 
== Sklici in opombe ==
 
{{sklici|3}}
 
== Viri ==
Z izračunom dobimo frekvenco vrha sevanja, ki znaša 46,9 terahercov (THz), kar se nahaja ravno na prehodu iz infrardečega spektra sevanja v slabo vidno temno rdečo barvo.<ref>{{cite book | title = Biology: Concepts and Applications | author = Starr, C. | publisher = Thomson Brooks/Cole | year = 2005 | isbn = 0-534-46226-X | url = http://books.google.com/books?id=RtSpGV_Pl_0C&pg=PA94}}</ref>
 
|* author{{navedi revijo|last1= Draper,|first= J.W.John William|authorlink1= John William Draper|title = On the Production of Light by Heat|journal = The London, Edinburgh and Dublin philosophical magazine and journal of science| year = 1847| page = 345&ndash;359| url = http://books.google.com/books?id=VEgEAAAAYAAJ&pg=PA345|ref= harv}}</ref>
== Sklici in opombe ==
* {{navedi knjigo|last1= Mahan|first1= J. Robert|title = Radiation heat transfer: a statistical approach|edition = 3|publisher = Wiley-IEEE|year = 2002|isbn = 978-0-471-21270-6|page = 58|url = http://books.google.com/books?id=y9zUEzA7iN0C&pg=PA58&dq=draper-point+red&lr=&as_drrb_is=q&as_minm_is=0&as_miny_is=&as_maxm_is=0&as_maxy_is=&as_brr=3&ei=H8ttSo_2LImMkQTwvuxO|ref= harv}}
{{opombe}}
* {{navedi revijo|last1= Murray|first1= J.|journal = [[The Academy]]|title = Science: Draper's Memoirs|volume = XIV|issue = 338|date = 1878|page = 408|url= http://books.google.com/books?id=hZINAAAAQAAJ&pg=PA408&dq=draper+point+red+1847&lr=&as_brr=0&ei=6sxtSpnpLoLglATlh4RW|ref= harv}}
* {{navedi knjigo|last1= Starr|first1= Cecie|title = Biology: Concepts and Applications|publisher = Thomson Brooks/Cole|year = 2005|isbn = 0-534-46226-X|url = http://books.google.com/books?id=RtSpGV_Pl_0C&pg=PA94|ref= harv}}
* {{navedi knjigo|last1= Wannier|first1= Gregory Hugh|authorlink1= Gregory Hugh Wannier|title= Statistical Physics|year= 1987|origyear= 1966|publisher= Dover Publications|location= New York|isbn= 978-0-486-65401-0|oclc= 15520414|chapter= Chapter 10-2|ref= harv}}
 
{{fizikalna škrbina}}