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October 2, 2024 Solar Eclipse Times Event Time (UTC) First Penumbral External Contact 2024 October 02 at 15:44:08.1 UTC First Umbral External Contact 2024 October 02 at 17:32:12.9 UTC First Central Line 2024 October 02 at 16:54:48.8 UTC First Umbral Internal Contact 2024 October 02 at 16:57:52.5 UTC First Penumbral Internal Contact
PM Surya Ghar Muft Bijli Yojana is a scheme launched by the Government of India in its 2024-25 budget for rooftop solar plant project with an investment of over 75,000 crore rupees to provide solar power for about 1 crore households and to provide them 300 units of free electricity every month.
Rahu's head was exiled to the heavens, and due to the two celestial deities' part in his decapitation, he is said to occasionally swallow them whole for a given period of time, causing the solar and the lunar eclipse. [5] in other texts, the eclipse is associated with Svarbhanu, who is sometimes identified as the asura whose head became Rahu.
As the magnitude of this eclipse at that time was 1.0566, the angular diameter of the Moon was 1.0566 times that of the Sun, or 33'44". This gave the eclipse a wider path of totality and more maximum time in totality (4 min 28 s) compared to the total eclipse in 2017 (2 min 40 s), which had a magnitude of 1.0306.
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Of these, two annular and one total eclipse will be non-central, [1] in the sense that the very center (axis) of the Moon's shadow will miss the Earth (for more information see gamma). [2] In the 21st century, the greatest number of eclipses in one year is four, in 2011, 2029, 2047, 2065, 2076, and 2094.
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially.Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to the plane of Earth's orbit. [1]
The nirayana year is the sidereal year, that is, is the actual time required for the Earth to revolve once around the Sun with respect to a fixed point on the ecliptic, and its duration is approximately 365.256363 days (365 days 6 hours 9 minutes 10 seconds).