1,600
After 6 years, approximately 5 grams of cesium-137 would remain from a 10 g sample due to its half-life of around 30 years. This decay is exponential, with about half of the original sample decaying every 30 years.
After 4.47 billion years, roughly half of the original atoms of uranium-238 would have decayed to lead-206 through alpha decay. This means there would be about 30 atoms of uranium-238 remaining.
The Earth has been habitable for living organisms for about 3.5 billion years.
Hydrocarbons are composed of hydrogen and carbon atoms. These atoms can form various types of bonds, resulting in different classes of hydrocarbons such as alkanes, alkenes, and alkynes. The structures and properties of hydrocarbons depend on the specific arrangement of carbon and hydrogen atoms.
Photosynthetic organisms, such as cyanobacteria, are believed to have appeared around 3.5 billion years ago. These early organisms played a crucial role in shaping Earth's atmosphere by producing oxygen as a byproduct of photosynthesis.
The half-life is 5730. This is because the half-life is the amount of time it takes for half of a sample to decay. In this case, the sample is 100 atoms, and half of 100 is 50, so the amount of time it takes the sample to reach 50 atoms is it's half life...5730!
5730 years (approx).
1.25 billion years
The half-life of potassium-40 is 1.25 billion years since half of the original sample decays in that time. With 50 atoms initially, having 25 atoms remaining after 1.25 billion years aligns with the expected decay pattern for a half-life.
The half-life is 5730. This is because the half-life is the amount of time it takes for half of a sample to decay. In this case, the sample is 100 atoms, and half of 100 is 50, so the amount of time it takes the sample to reach 50 atoms is it's half life...5730!
The half-life of carbon-14 is 5 730 years.
To calculate the evaporation rate, we need to know the number of atoms in the sample. The number of atoms in a 2 ml sample of liquid mercury can be calculated using Avogadro's number (6.022 x 10^23 atoms/mol for mercury). Then, divide the total number of atoms by the total number of seconds in 25 years to get the evaporation rate in atoms per second.
700 milliion years. The definition of half-life is the period of time during which one-half of the atoms of an element undergo decay into other elements.
1.25 billion years: 25/50 or half the original atoms have disintegrated in 1.25 billion years, and that is the definition of half life.
Half-life of 2000 years means that after 2000 years, half of the sample will decay - so of course the other half of the sample is still around.Half-life of 2000 years means that after 2000 years, half of the sample will decay - so of course the other half of the sample is still around.Half-life of 2000 years means that after 2000 years, half of the sample will decay - so of course the other half of the sample is still around.Half-life of 2000 years means that after 2000 years, half of the sample will decay - so of course the other half of the sample is still around.
A Sample Of Zircon 35 Atom Of 207Pb for every 5 atoms of 235U. How Old Is Zircon? t(1/2)=5730. K=0.693/704E6=9.8E-10 -1/K ln(5/90)= years
The half-life of rubidium-87 is approximately 48.8 billion years. This means it would take about 48.8 billion years for half of the rubidium-87 atoms in a rock sample to decay into strontium-87. Therefore, to see half of the rubidium-87 atoms change into strontium-87, you would need to wait this extensive period.