About 448 minutes
Side-Lights on Astronomy and Kindred Fields of Popular Science — Story, Setting & Ideas
Popular Astronomy
103,032 recorded words. 6 minutes difference from this book's estimate.
View Gutenberg source #4065The source record for Astronomy of To-day: A Popular Introduction in Non-Technical Language — A Reader’s Guide measures this digital text at 104,254 words, 7 hr 34 min estimated reading time, and 19 detected text sections.
The text analysis averages about 21.1 words per sentence, while the detected sections provide another way to judge how the source is divided.
Project Gutenberg metadata also associates the work with “Astronomy,” connecting these edition facts with the source record’s subject description.
Explore this collection
These alternatives are selected using recorded categories and estimated reading time.
About 448 minutes
Popular Astronomy
103,032 recorded words. 6 minutes difference from this book's estimate.
View Gutenberg source #4065About 494 minutes
Popular Astronomy
113,513 recorded words. 40 minutes difference from this book's estimate.
View Gutenberg source #28613About 364 minutes
Popular Astronomy
83,582 recorded words. 90 minutes difference from this book's estimate.
View Gutenberg source #58810Search stored excerpts and compare books → Choose by your preferences →
Choices use stored catalog measurements. Estimates vary with reading speed. A shared category is a catalog label, not a claim that two books have the same argument or literary quality.
Search reads excerpt text stored with this catalog and links to its associated Gutenberg record. The connection is stored in the site database; this tool does not recheck that every excerpt is word-for-word identical to that external record. Excerpt search does not cover every chapter and does not verify historical publication dates.
Catalog snapshot checked: 2026-09-26. Coverage: 85 public books, 83 available source excerpts.
Calculated from edition completeness, EPUB availability, text structure and catalogue metadata. Not a user rating.
Total of 100 points, scaled to a 2.5-5.0 range. Editions with an empty description or a missing EPUB file are not scored.
Public-domain source text
The source text is kept in the dedicated reader, separate from this catalogue record and its commentary.
Cecil G. Dolmage's Astronomy of To-day (1910) opens with a clear mission: to present astronomical facts and theories in the ordinary language of everyday life, avoiding the mathematical forms that repel the general reader. The preface positions diagrams as self-contained pictorial aids, not cross-referenced to the text, and the coloured frontispiece as art distinct from science. This deliberate separation of visual and verbal explanation shapes the book's accessible approach.
Dolmage explicitly addresses the barrier mathematics poses to popular astronomy. He describes mathematical processes as no more than ordinary logic in concentrated form, calling them the shorthand of reasoning. This framing allows him to present main facts and theories without equations, relying instead on verbal explanation and supplementary diagrams. The preface insists that reasoning about celestial orbs is of no different order from everyday affairs, a claim that invites the general reader to engage without specialized training.
The book's structure reflects this commitment: diagrams are not linked by wearying cross-references but are complete in themselves. This design choice minimizes interruption and lets the text flow conversationally. Dolmage's tone throughout the excerpts remains explanatory rather than technical, consistent with his stated goal of making astronomy accessible to a broad audience.
The excerpts on Mars reveal a nuanced treatment of the canal debate, a topic that had captured public imagination. Dolmage presents Percival Lowell's theory that the straight lines and geometric arrangement of Martian canals indicate artificial irrigation by intelligent inhabitants. He notes that Lowell's views are not wild but are called forth by remarkable observations. The liquid from melting polar caps appears to travel toward the equator and then to the opposite pole, a process Lowell argues must be helped artificially, as by pumping.
However, Dolmage also gives substantial space to skeptical perspectives. He describes experiments by Maunder and Evans in 1902, where schoolboys at varying distances from a disc with faint markings produced drawings that supported the idea that the eye may unconsciously connect point-like markings into lines near the limit of visibility. He then reports that photographs from the 1905 opposition, taken by Lampland at Lowell Observatory, showed several prominent canals as straight dark lines, and later photographs even suggested doubling. Dolmage presents both sides without endorsing either, leaving the reader to weigh the evidence.
Dolmage's preface indicates that the book contains incidental matter concerned with the astronomy of the past, introduced to clarify present understanding. The excerpts do not reveal how extensively historical material appears, but the approach suggests a progressive narrative from earlier ideas to contemporary knowledge. The author's careful hedging—phrases like it is said, appears, and seems a strong point—reflects a cautious empiricism.
Notably, Dolmage refrains from claiming definitive proof for any theory about Mars. He explicitly states that a great deal of nonsense has been written in newspapers about life on Mars, and that no actual evidence of living beings exists. This restraint contrasts with the sensationalism of popular press accounts, positioning the book as a sober corrective. The excerpts do not reveal whether Dolmage ultimately favors Lowell's irrigation hypothesis or the optical illusion explanation; he presents the debate as ongoing, with photographs beginning to tip the scales but not conclusively.
Readers should approach Astronomy of To-day as a snapshot of early twentieth-century popular science, where the author's commitment to non-technical language coexists with unresolved scientific controversies. The Martian canal discussion exemplifies how Dolmage balances competing hypotheses without oversimplifying. Those interested in the history of astronomy or the public understanding of science will find this work a valuable primary source, revealing both what was known and what was debated in 1910.
Holding this 1910 volume, I recalled evenings spent tracing canal lines in my own childhood atlas, wondering at Lowell’s certainty. That same quiet awe returned with Astronomy for Young Folks — Reading Notes years later—not for answers, but for how both books let a beginner simply look up and feel small, yet part of something vast.
Save your reaction, strongest insight, and memorable passage.