Here I have collected real errors in the book by Jack B. Zirker "Journey from the Center if the Sun", 1st edition, Princeton University Press, 2002 H.Woehl, last update (typing error corrected): March 24, 2006 1) ch.2, page 18: The detection of the spectral lines in the solar spectrum in 1802 should be credited to W.H. Wollaston (1766-1828) instead of J.Fraunhofer, who found the lines only in 1814. Correct is that Wollaston detected only the strongest, while Fraunhofer counted about 500 absorption lines. 2) ch.4, page 58 bottom and Fig.4.3 on page 59, top: The "size" of granules should better be given as its "diameter" ? - Worse is that their lifetime is given as "about eight or ten minutes" in the text and "last for 5 minutes" in the caption to the figure. In fact large granules have lifetimes up to 20 minutes and smaller granules can dissolve even after less than 5 mintes. 3) ch.4, pages 59-61: The Benard cells in laboratory experiments depend not just on the convection, but mainly on surface tension. It's not just the difference in Rayleigh numbers that counts. 4) ch.4, pages 65-67 and Fig.4.6: Neither in the text nor in the caption to the figure the scale of the subimages is given. I guess it is a few 1000 km. It would also to be helpfull to have an idea about the gray-scale-coding, either by a 'code bar' transforming grey-scales to values or at least by the minima and maxima in each subimage...In addition: its again a terrible grey-scale image for me. 5) ch.5, page 83, 15th line from the bottom: There is a reference given to Figure 5.9, it should read 5.8 6) ch.5, page 84, 4th line from the bottom: It is unclear whether the old Figure 5.8, cited here was skipped, because the caption of Fig.5.8 indicate data of Grec and Fossat, not of the Birmingham group... 7) ch.6, page 99, 8th line from the top: The granules, each as large as Brazil, packed edge to edge... - The mean diameter of granules is about 1000 km - Brazil or Alaska (cited in chapter 1, page 12 in the caption to Fig.1.7 and in chapter 4, page 58, 5th line from the bottom) - are both larger and Brazil is even about 5 times as large as Texas...In addition there is an intergranular net between the granules, so they are not really "packed edge to edge". See e.g. the Fig. 4.3, page 59 - although its a rather bad image by todays standards. 8) ch.6, page 102,at the bottom: See remark (1) - the credit for the detection is now given to Wollaston, but the year is wrong, instead of 1814 it should read 1802. 9) ch.7, page 120, bottom: It was not "just as a hobby", that Schwabe started to observe sunspots, but he was searching for a planet between Mercury and the sun, the famous 'Vulcan'. As many astronomers of his time expected, such a planet could be detected during the passage on the disk of the sun...[See the biographies of Schwabe, e.g. in the INTERNET: http://www.plicht.de/chris/32schwab.htm] 10) ch.7, page 138 : There are two famous sites on the Canary Island: The one mentioned in the text is on the most western of the group of islands. Its name is "La Palma". The french-italian telescope THEMIS is not there ! It stands nearby the german Vacuum Tower Telescope on the main Canary Island called "Tenerife". For details of the site selection for solar telescopes on the Canary Islands see e.g.: Brandt and Woehl: Astron.Astrophys. 109, 77 (1982). 11) ch.9, Fig. 9.7: There is no information given about the wavelengths of light in which this image of a sunspot was taken. I doubt it was in "white light" - maybe H alpha ? 12) ch.9, page 164, line 2: When a fact was reported more than 20 years ago, its not "recent" in scientific publication standards: See the report about sunspot contrasts by Albregtsen, F., Maltby, P. in Solar Physics, vol. 71, June 1981, p. 269-283 13) ch.12, page 231, 14th line from the bottom: Figure 11.8 is a model of the "magnetic carpent", maybe the author refers to Fig.11.4 here - again one of very poor quality...Hopefully O.Engvold had better examples available when examing the movies of R.Dunn... 14) ch.13, page 237, middle: H.Schwabe observed the sunspots very frequently from 1826 until 1843 and then announced a period of the sunspot cycle of 10 years.