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What is the value of angular momentum of electron in second excited state of hydrogen atom as per Bohr’s model?
The angular momentum of an electron in the second excited state (n=3) of a hydrogen atom, according to Bohr's model, is given by L = nℏ, where n = 3. Thus, L = 3ℏ. For more visit here: https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-12/
The angular momentum of an electron in the second excited state (n=3) of a hydrogen atom, according to Bohr’s model, is given by L = nℏ, where
n = 3. Thus, L = 3ℏ.
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According to kinetic theory of gases at absolute zero of temperature
According to the kinetic theory of gases, at absolute zero (0 Kelvin or -273.15°C), the molecules of a substance have no kinetic energy and their motion theoretically stops completely. This is the lowest possible temperature. Click this more information: https://www.tiwariacademy.com/ncert-solutionsRead more
According to the kinetic theory of gases, at absolute zero (0 Kelvin or -273.15°C), the molecules of a substance have no kinetic energy and their motion theoretically stops completely. This is the lowest possible temperature.
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Mercury thermometer can be used to measure temperature upto
Mercury thermometers can measure temperatures up to around 360°C because mercury stays in its liquid state up to this temperature. Beyond this, mercury begins to vaporize and cannot be used for measurements above this point. Click for more: https://www.tiwariacademy.com/ncert-solutions/class-11/physRead more
Mercury thermometers can measure temperatures up to around 360°C because mercury stays in its liquid state up to this temperature. Beyond this, mercury begins to vaporize and cannot be used for measurements above this point.
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If the temperature of the sun were to increase from T to 2 T and its radius from R to 2 R, then the ratio of the radiant energy received on earth to what it was previously, will be
The amount of sun's radiant energy received is proportional to the power output of the sun from Stefan-Boltzmann's Law: P ∝ R²T⁴ 1. Preliminary P₁ ∝ R²T⁴ 2. After alteration - The radius increases to 2R: The area increases proportionally to (2R)² = 4R² - Temperature increases to 2T: Power increasesRead more
The amount of sun’s radiant energy received is proportional to the power output of the sun from Stefan-Boltzmann’s Law:
P ∝ R²T⁴
1. Preliminary
P₁ ∝ R²T⁴
2. After alteration
– The radius increases to 2R: The area increases proportionally to (2R)² = 4R²
– Temperature increases to 2T: Power increases proportionally to (2T)⁴ = 16T⁴
– Total power increases to:
P₂ ∝ 4R² × 16T⁴ = 64R²T⁴
3. The ratio of the new power to the old power:
P₂ / P₁ = (64R²T⁴) / (R²T⁴) = 64
Thus, the radiant energy received on Earth will increase by a factor of 64.
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What did you enjoy doing?
I enjoyed the hands-on experience of planting seeds, nurturing them with care, and witnessing their growth. Watering the plants and maintaining the garden offered a sense of responsibility and satisfaction. The highlight was harvesting fresh produce, which was a rewarding outcome of the effort. AddiRead more
I enjoyed the hands-on experience of planting seeds, nurturing them with care, and witnessing their growth. Watering the plants and maintaining the garden offered a sense of responsibility and satisfaction. The highlight was harvesting fresh produce, which was a rewarding outcome of the effort. Additionally, designing the garden layout, arranging pots, and adding decorative elements enhanced the joy of the activity, making it both educational and creatively fulfilling.
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