You can use the concepts in this chapter to obtain an estimate of the number of atoms in the universe. These steps will guide you through this calculation. (a) Begin by calculating the number of atoms in the sun. Assume that the sun is pure hydrogen with a density of 1.4 g>cm3 . The radius of the sun is 7 * 108 m, and the volume of a sphere is V = 4 3pr3 . (b) The sun is an average-sized star, and stars are believed to compose most of the mass of the visible universe (planets are so small they can be ignored), so we can estimate the number of atoms in a galaxy by assuming that every star in the galaxy has the same number of atoms as our sun. The Milky Way galaxy is believed to contain 1 * 1011 stars. Use your answer from part a to calculate the number of atoms in the Milky Way galaxy (c) Astronomers estimate that the universe contains approximately 1 * 1011 galaxies. If each of these galaxies contains the same number of atoms as the Milky Way galaxy, what is the total number of atoms in the universe?

Short Answer

Expert verified
To estimate the number of atoms in the universe, calculate the number of atoms in the sun using its volume and density, then multiply by the number of stars in the Milky Way, and finally by the estimated number of galaxies in the universe.

Step by step solution

01

Calculate the volume of the sun

First, calculate the volume of the sun using the volume formula for a sphere, which is \( V = \frac{4}{3}\pi r^3 \). Plug in the radius of the sun, \(7 \times 10^8\) meters, into the formula to find the volume.
02

Convert the volume to cubic centimeters

Since the density is given in grams per cubic centimeter, we must convert the volume from cubic meters to cubic centimeters. To do this, we use the conversion factor \(1 m^3 = 10^6 cm^3\).
03

Calculate the mass of the sun

Multiply the volume of the sun in cubic centimeters by the density of hydrogen, which is \(1.4 g/cm^3\), to obtain the sun's mass in grams.
04

Calculate the number of atoms in the sun

Hydrogen has an atomic mass of approximately 1 gram per mole, and one mole of any element contains Avogadro's number of atoms \(6.022 \times 10^{23}\). Divide the sun's mass by the atomic mass of hydrogen to get the number of moles of hydrogen in the sun, and then multiply by Avogadro's number to find the total number of atoms.
05

Calculate the number of atoms in the Milky Way galaxy

The Milky Way galaxy is believed to contain \(1 \times 10^{11}\) stars. Multiply the number of atoms in one sun (from Step 4) by the number of stars in the Milky Way to estimate the total number of atoms in the galaxy.
06

Estimate the total number of atoms in the universe

Astronomers estimate that there are \(1 \times 10^{11}\) galaxies in the universe. Multiply the total number of atoms in one galaxy (from Step 5) by the number of galaxies to estimate the total number of atoms in the universe.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Atomic Mass and Moles
Understanding the relationship between atomic mass and moles is crucial for estimating the number of atoms in a substance. The atomic mass, often referred to as the atomic weight, is essentially the mass of an atom expressed in atomic mass units (amu). Hydrogen, for instance, has an atomic mass of approximately 1 amu, or 1 gram per mole.

A mole is a unit of measurement that represents a quantity of particles, such as atoms. Avogadro's number, which is approximately \(6.022 \times 10^{23}\), defines the number of particles in a mole. In our context, since atomic mass and moles are directly related, you can find out the number of moles in the sun by dividing its mass by the atomic mass of hydrogen, and then calculate the total number of atoms by multiplying the moles by Avogadro's number.
Volume Calculation of Spheres
To estimate the number of atoms in the sun, it's essential to first calculate its volume as it is a near-perfect sphere. The volume of a sphere is determined by the formula \( V = \frac{4}{3}\pi r^3 \), where \( r \) is the radius of the sphere. For the sun, with radius \(7 \times 10^8\) meters, this equation can be used to ascertain the volume in cubic meters.

Understanding the geometry of spheres and how to apply this formula is a staple in physics and astronomy, as it allows us to calculate space occupied by celestial bodies. This volume can later be used, combined with density, to find the mass, a stepping stone in our journey to counting atoms.
Converting Volume Units
When the volume of the sun is calculated, it's in cubic meters. However, density of hydrogen given for our calculations is in grams per cubic centimeter. To keep units consistent for mass calculations, the volume must be converted using the factor \(1 m^3 = 10^6 cm^3\).

This conversion is pivotal because it aligns the volume units with the density units, enabling the calculation of the mass of the sun in grams—a key metric for finding the number of atoms within.
Density and Mass Relationship
Density is defined as mass per unit volume and is a measure of how much matter is packed into a given space. By multiplying the density of an object by its volume, one can calculate its mass.

In the case of the sun, if we assume it's composed of pure hydrogen with a density of \(1.4 g/cm^3\), and we've converted its volume to cubic centimeters, we can find its mass. This mass holds all the hydrogen atoms we're trying to estimate, revealing the close ties between density, volume, and mass in astrophysical contexts.
Avogadro's Number
Avogadro's number is a consistent value used in chemistry to denote the number of constituent particles, usually atoms or molecules, in one mole of a given substance. Being a fundamental constant of nature, \(6.022 \times 10^{23}\) is a way to bridge the microscopic world of atoms with the macroscopic data we can measure, such as grams per mole.

It transforms the mass of the sun, or any other celestial object into a count of atoms, building a bridge from tangible measurements to the number of fundamental particles they contain, a necessary step for estimating atoms in the universe.
Astronomical Estimates of Stars and Galaxies
The universe is a vast expanse, containing an immense number of galaxies, which themselves harbour billions of stars. Astronomical estimates suggest about \(1 \times 10^{11}\) galaxies are in the observable universe, each with its own plethora of stars. Using our Milky Way as a baseline, with an estimated \(1 \times 10^{11}\) stars, illustrates the scale at which cosmologists work when making such estimates.

The enormity of these numbers can be challenging to comprehend, but by assuming that each star has roughly the same number of atoms as our sun and then multiplying this by the number of stars in a galaxy—and then by the number of galaxies—we can approximate the total number of atoms in the universe, showcasing the blend of astronomical observation with atomic-scale calculation.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Study anywhere. Anytime. Across all devices.

Sign-up for free