Errata in Essential Astrophysics
I’ve adopted Kenneth Lang’s Essential Astrophysics for my ASTRO 320 class at U. Alberta this year. It has the wonderful feature of being relatively low cost owing to the University Library subscribing to the Springer eBooks. Thanks, Library. Unfortunately, the book is a First Edition. As such there are typos. Here is a list of the ones we’ve found so far.
Section 2.4, Page 45
The Planck function (Eq. 2.17) is given as
where it should be
Section 2.4, Page 45
The value of is given as 3.13159 and should be 3.14159.
Section 2.4, Page 46
The Planck function (Eq. 2.18) is given as
where it should be
Section 2.4, Page 48
The radiation energy (Eq. 2.23) density
should read
Section 2.4, Page 49
Above Equation 2.29, the text says “energy flowing out of the blackbody over sr, or over the hemisphere facing an observer.”
A hemisphere is sr, but the equation is correct. The “missing” factor of comes from the shrinking projected size of the differential area at larger angles.
Section 2.4, Page 50
The Stefan-Boltzmann Constant is given as and it should be . (Thank you Tanner S.)
Focus 2.5, Page 59
Dr. Hans Seuss died in 1993 not 1920, which makes his story a lot less about tragic death at an early age. (Thanks to Paul).
Section 5.4.1, Page 141
The book gives the solar wind pressure as a “startling Pa,” which would be truly startling and would also deliver enough energy to destroy the planet in a year. The actual numbers that NOAA bandies about are closer to Pa.
Section 6.3, Page 174
Boltzmann was born in 1844 not 1894, which Michelle S. noted the date in the text would be hard to reconcile with Boltzmann deriving his eponymous distribution in 1872.
Section 8.3.3, Page 232
An MeV is not 1.692 as given at the bottom of the page.
Section 10.1.2, Page 296
The magnitude system is defined so that an interval of five magnitudes correspond to exactly a factor of 100 in brightness. Thus, Equation 10.4 should read
Section 10.5.6, Page 354
The first generation of stars is broadly described as Population III and theoretically had . The second, slightly enriched generation was called Population II, which are relatively metal-poor compared to most stars (). Finally, most stars seen today have roughly solar metallicity () and are called Population I.