it s 3050
Mass
One method to determine the mass of each star in a binary star system is by studying their orbital motion. By observing the period and separation of the stars' orbits, astronomers can calculate the masses using Kepler's laws of planetary motion and Newton's law of universal gravitation.
You need its mass and volume.
The mass/luminosity relation is important because it can be used to find the distance to binary systems which are too far for normal parallax measurements.
Two measurements needed to determine density are the mass of the object and its volume. Mass can be measured using a scale, while volume can be measured using a ruler or by water displacement method. Density is calculated by dividing the mass of the object by its volume.
If you're talking about mass spectrometry, the measurements made for each isotope during the detection process are abundance and mass to charge ratio.
You can use mathematical formulas to determine measurements of mass, force, weight, wavelength, etc.
You need to know two of them - either from your own or other people's measurements. The third can then be determined using Density = Mass/Volume
The average stellar mass x the number of stars ______________________________ We can calculate the mass of the Milky Way by observing the speed at which stars orbit the center, as long as we can determine how far away they are from the center.
To determine the density of a substance, you would divide the mass of the substance by its volume. The formula for density is density = mass/volume. Measurements should be taken in units such as grams for mass and cubic centimeters for volume.
Mass percentage calculations determine the percentage of an element based on mass in a compound. This can then be used to determine the percentage in a compound of each individual element.
The correct measurement will likely be the average of multiple measurements taken for the feather's mass. This helps to account for any errors or inconsistencies that may occur during the measurements.