2.6 Useful Measurements in Astronomy

In astronomy we deal with distances on a scale you may never have thought about before, with numbers larger than any you may have encountered. We adopt two approaches that make dealing with astronomical numbers a little bit easier. First, we use a system for writing large and small numbers called scientific notation (or sometimes powers-of-ten notation). This system is very appealing because it eliminates the many zeros that can seem overwhelming to the reader. In scientific notation, if you want to write a number such as [latex]500,000,000[/latex], you express it as [latex]5\times 10^8[/latex]. The small raised number after the [latex]10[/latex], called an exponent, keeps track of the number of places we had to move the decimal point to the left to convert [latex]500,000,000[/latex] to [latex]5[/latex]. The second way we try to keep numbers simple is to use a consistent set of units—the metric International System of Units, or SI (from the French Système International d’Unités).

A common unit astronomers use to describe distances in the universe is a light-year, which is the distance light travels during one year. Because light always travels at the same speed, and because its speed turns out to be the fastest possible speed in the universe, it makes a good standard for keeping track of distances. You might be confused because a “light-year” seems to imply that we are measuring time, but this mix-up of time and distance is common in everyday life as well. For example, when your friend asks where the movie theater is located, you might say “about [latex]20[/latex] minutes from downtown.”

So, how many kilometres are there in a light-year? Light travels at the amazing pace of [latex]3\times 10^5[/latex] kilometres per second (km/s), which makes a light-year [latex]9.46\times 10^{12}[/latex] kilometres. You might think that such a large unit would reach the nearest star easily, but the stars are far more remote than our imaginations might lead us to believe. Even the nearest star is [latex]4.3[/latex] light-years away—more than [latex]40[/latex] trillion kilometres. Other stars visible to the unaided eye are hundreds to thousands of light-years away as seen in Figure 2.1.

Orion Nebula

Photograph of the Orion Nebula. This image is dominated by large areas and bright swirls of glowing gas clouds, crisscrossed by dark bands of dust.
Figure 2.1. This beautiful cloud of cosmic raw material (gas and dust from which new stars and planets are being made) called the Orion Nebula is about 1400 light-years away. That’s a distance of roughly 1.34 × 1016 kilometres—a pretty big number. The gas and dust in this region are illuminated by the intense light from a few extremely energetic adolescent stars.
Hubble’s Sharpest View of the Orion Nebula by NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team, NASA Media Licence.
Table 2.4 Astronomical Constants
Name Value
speed of Light (c) [latex]3\times 10^5\;\text{km/s}[/latex]
astronomical unit (AU) [latex]1.496\times 10^{11}\;\text{m}[/latex]
light-year (ly) [latex]9.461\times 10^{15}\;\text{m}[/latex]
parsec (pc) [latex]3.086\times 10^{16}\;\text{m}=3.262\;\text{light-years}[/latex]
sidereal year (y) [latex]3.156\times 10^7\;\text{s}[/latex]
mass of Earth ([latex]M_\textrm{Earth}[/latex]) [latex]5.974\times 10^{24}\;\text{kg}[/latex]
equatorial radius of Earth ([latex]R_\textrm{Earth}[/latex]) [latex]6.378\times 10^6\;\text{m}[/latex]
obliquity of ecliptic [latex]23.4^{\circ} 26’[/latex]
surface gravity of Earth ([latex]g[/latex]) [latex]9.807\;\text{m/s}^2[/latex]
escape velocity of Earth ([latex]V_\textrm{Earth}[/latex]) [latex]1.119\times 10^4\;\text{m/s}[/latex]
mass of Sun ([latex]M_\textrm{Sun}[/latex]) [latex]1.989\times 10^{30}\;\text{kg}[/latex]
equatorial radius of Sun ([latex]R_\text{Sun}[/latex]) [latex]6.960\times 10^8\;\text{m}[/latex]
luminosity of Sun ([latex]L_\textrm{Sun}[/latex]) [latex]3.85\times 10^{26}\;\text{W}[/latex]
solar constant (flux of energy received at Earth) (S) [latex]1.368\times 10^3\;\text{W/m}^2[/latex]
Hubble constant (H0) approximately [latex]20[/latex] km/s per million light-years, or approximately 70 km/s per megaparsec

Attribution

1.4 Numbers in Astronomy and Scientific Notation or Powers of Ten” and “A.5 Some Useful Constants for Astronomy” from Douglas College Astronomy 1105 by Douglas College Department of Physics and Astronomy, are licensed under a Creative Commons Attribution 4.0 International License, except where otherwise noted. Adapted from Astronomy 2e.

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Fanshawe College Astronomy Copyright © 2023 by Dr. Iftekhar Haque is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License, except where otherwise noted.