location, place, human-environment interaction, movement and region.
Marselie, provence-alpes-côte d'azur
Answer:
About 16 times the energy of the second.
Explanation:
This can be explained thanks to the Stefan-Boltzmann law, which relates temperature directly to the amount of energy released by an object.
With this law in mind, the total energy radiated during 1 second from 1 square meter of any object, equals <em>a constant </em>(5.670374419 × 10−8 watt per meter2 per K4) times the temperature raised to the fourth power. the equation is:
E = σT4
Since the first star is twice as hot as the second, then the star won't produce twice the energy, but 16 times the energy due to the Stefan-Boltzmann constant. It's also important to know that this law only applies to blackbodies.
Answer: The Government of India Act 1935 was an Act of the Parliament of the United Kingdom.
Explanation: It originally received Royal assent in August 1935 (25 & 26 Geo. 5 c. 42). Until 1999, it was the longest Act (British) of Parliament ever enacted. At that time, the Greater London Authority Act 1999 surpassed it in length. Because of its length, the Act was retroactively split by the Government of India Act, 1935 (Re-printed) (26 Geo. 5 & 1 Edw. 8 c. 1) into two separate Acts:
1. The Government of India Act, 1935 (26 Geo. 5 & 1 Edw. 8 c. 2), having 321 sections and 10 schedules.
2. The Government of Burma Act, 1935 (26 Geo. 5 & 1 Edw. 8 c. 3), having 159 sections and 6 schedules.
References in the literature on Indian political and constitutional history are usually to the shortened Government of India Act, 1935 (i.e. 26 Geo. 5 & 1 Edw. 8 c. 2), rather than to the text of the Act as originally enacted.
