The Story of the Solar System — Inside the Classic

A Practical Telescope Companion

Chambers frames his book for owners of popular telescopes costing between £10 and £50, insisting that patience and perseverance matter more than aperture. He counters the “extremely common” notion that a big telescope is necessary by pointing to Goldschmidt’s attic-window discoveries. This practical bent shapes the entire work: the reader is assumed to be an observer, not merely a reader of summaries. The preface’s tone is collegial yet firm, warning against “croakers” who dismiss small instruments. Later excerpts, such as the discussion of lunar heat and cloud dispersal, reinforce this observational stance by weighing personal experience against statistical arguments.

Lunar Influences and Skeptical Statistics

In the chapter on the Moon, Chambers presents a detailed case for lunar effects on terrestrial clouds, citing Sir John Herschel’s “tendency to disappearance of clouds under a full Moon.” He acknowledges counter-evidence from Mr. Ellis of the Royal Observatory but dismisses it with a tart remark: “you can prove anything you like by statistics.” Chambers then asserts his own conviction, based on “more than 30 years’ observation,” that clouds do disperse near the meridian full Moon. He also references Humboldt and Arago, but firmly rejects the popular notion that weather changes predictably at the Moon’s “changes,” calling such tables “void of authority.” This section reveals Chambers as an empiricist who trusts his own eyes over statistical arrays.

Orbital Precision and Descriptive Restraint

Despite his disdain for “mere figures,” Chambers supplies precise orbital data: the Moon’s revolution period of “27 d. 7 h. 43 m. 11 s.,” mean distance 237,300 miles, and diameter 2,160 miles. He notes the angular diameter at mean distance is “31′ 5″.” These numbers are embedded in flowing prose, not tables, consistent with his aim for “general reading.” The description of the Moon’s orbit as “somewhat, but not very, eccentric” typifies his measured language. He avoids dramatic claims, even when discussing lunar heat: he reports F. W. Very’s “heat-gradient” idea and Lord Rosse’s observations without overstatement. This restraint gives the book a reliable, almost legal tone—fitting for a barrister.

The Authorial Voice: Barrister and Astronomer

Chambers’ title page identifies him as “F.R.A.S. of the Inner Temple, Barrister-at-Law,” and his writing reflects that dual identity. He structures arguments like a case: stating a proposition (clouds disperse under full Moon), presenting opposing evidence (Ellis’s statistics), then delivering his own conclusion based on long observation. He uses legal phrasing such as “void of authority” and “if such a phrase is admissible.” The preface’s borrowing from Green’s Making of England shows a historian’s care for attribution. This voice—authoritative yet conversational, precise yet personal—distinguishes the book from dry textbooks. Readers should expect reasoned advocacy rather than neutral exposition.

Chambers’ Story of the Solar System rewards readers who approach it as a seasoned observer’s companion rather than a modern astronomy primer. The author’s willingness to challenge statistical orthodoxy with personal experience invites critical engagement. For those using small telescopes, the book offers both practical encouragement and a model of patient, skeptical inquiry. The excerpts suggest that Chambers’ greatest value lies not in data—much of which is dated—but in his distinctive voice and observational philosophy.

Some evenings I set down Chambers' sturdy little guide and think how he trusted his own eyes over rumor. That same quiet confidence—amateur, unhurried, personal—lives on in Astronomy of To-day: A Popular Introduction in Non-Technical Language — A Reader’s Guide, as if one patient observer simply passed the torch to another across the years.