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This page describes an image कृष्णिका (ब्लॅकबॉडी) प्रारण

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Caption: वेगवेगळ्या तापमानाच्या ब्लॅकबॉडीजमधून उत्सर्जित रेडिएशनचे वक्र. x-अक्ष तरंगलांबी दर्शवतो आणि y-अक्ष प्रत्येक तरंगलांबीवर त्या ब्लॅकबॉडीच्या पृष्ठभागाच्या चौरस मीटरने प्रत्येक सेकंदाला उत्सर्जित होणारी ऊर्जा दर्शवितो. शरीर जितके गरम असेल तितकी तरंगलांबी कमी आणि निळा प्रकाश जास्तीत जास्त ऊर्जा उत्सर्जित करते. या प्लॉटमधील सर्वात थंड शरीर लाल प्रकाशात शिखरावर असूनही, इतर गरम शरीरे सर्वांत थंड शरीरापेक्षा जास्त लाल प्रकाश उत्सर्जित करतात.


Credit: अंतर्राष्ट्रीय खगोलीय संघ खगोलशास्त्र शिक्षण कार्यालय (IAU-OAE) - नियाल डिकॉन.

Diagram translation status: Not yet approved by a reviewer
Diagram translators: Kshitij Chavan
Related glossary terms: Wavelength , इलेक्ट्रोमॅग्नेटिक रेडिएशन (विद्युत चुंबकीय विकिरण) , कृष्णिका प्रारण
Categories: Physics

Created with support from: OAE Main Office Main Office

License: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) icons

Want to make your own version of this diagram? Then have a look at the code that produced this diagram on Github

In Other Languages

इंग्रजी: Blackbody Radiation
जर्मन: Schwarzkörperstrahlung
Portuguese BR: Radiação de corpo negro
Italian: Radiazione di corpo nero
French: Rayonnement du corps noir
अरेबिक: إشعاع الجسم الأسود
Simplified Chinese: 黑体辐射
Want to create your own translation? Then have a look at the code that produced this diagram on Github

The diagram captions presented on the OAE website were written, translated and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits for our translation project here. All media file captions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE". The media files themselves may have different licenses (see above) and should be credited as listed above under "credit".