The elements of starch are carbon, hydrogen, and oxygen.
Hydrogen (approximately 74%) and helium (approximately 24%) make up around 98% of the sun's composition. These elements are constantly undergoing nuclear fusion reactions in the sun's core, creating energy and enabling the sun to emit light and heat.
hydrogen mainly, but there undergo fission to form helium (which undergo fission as the star approaches supernova producing the heavy elements like carbon)
light is required by the plants to activate their chlorophyll smallest unit of light energy is a photon which also dissociates water molecules in a plant .this process is called photolysis which is used in production of starch
The Sun is primarily made up of hydrogen and helium, with smaller amounts of heavier elements such as carbon, oxygen, and nitrogen. These elements undergo nuclear fusion in the Sun's core to produce energy and light.
Period-1 represents elements of the sun. This period constitutes hydrogen and helium.
The elements within our own sun are as follows: Hydrogen 72.46 % Helium 25.85 % Oxygen 0.78 % Carbon 0.28 % Iron 0.16 % Sulfur 0.12 % Neon 0.12 % Nitrogen 0.09 % Silicon 0.07 % Magnesium 0.05 % The standard equation for starch is (C6H10O5)n, n being the number of those monomers is in the polymer. So, the ratio of elements in the Sun is approx. H: 100 to C: 1 to O: 1 The ratio of elements in starch is approx. H: 2 to C: 1 to O: 1. Significantly less elemental hydrogen exists in starch found on earth than on our own star.
the sun
hydrogen and helium
Hydrogen and helium.
helium
Most plants store energy in the form of starch. The process of photosynthesis allows plants to convert the sun's energy into glucose, which is then converted into starch. The plant can then break the starch back down whenever energy is needed.
Hydrogen (approximately 74%) and helium (approximately 24%) make up around 98% of the sun's composition. These elements are constantly undergoing nuclear fusion reactions in the sun's core, creating energy and enabling the sun to emit light and heat.
The Sun is primarily composed of hydrogen (74% by mass) and helium (24%). These two elements make up more than 98% of the Sun's total mass. Other elements like oxygen, carbon, neon, and iron make up the remaining portion in smaller quantities.
Many elements only form through high temperatures and pressures... both of which are present int the Sun - but not in the Earth's atmosphere.
Planets near the sun likely lost lighter elements like hydrogen and helium due to the sun's high temperature and solar wind. These elements were blown away, leaving behind the heavier elements that make up the terrestrial planets closer to the sun.
hydrogen mainly, but there undergo fission to form helium (which undergo fission as the star approaches supernova producing the heavy elements like carbon)
The Sun is primarily composed of hydrogen and helium, which make up about 74% and 24% of its mass, respectively. The remaining 2% consists of heavier elements such as oxygen, carbon, neon, and iron. These elements are crucial for the Sun's nuclear fusion processes, which generate the energy that powers the Sun and emits light and heat.