WCP2826

Letter (WCP2826.2716)

[1]1

ROYAL ASTRONOMICAL SOCIETY OF CANADA

Toronto Canada

May 22 [19]032

Dr Alfred Russel Wallace

Dear Sir:

I have read with pleasure your article on "Man’s Place in the Universe"3 also the criticism of the same by Prof[essor] W. H. Pickering4 Prof[essor] W. A. Maunder5 [sic], Prof[essor] Turner6 and Flammarion7. Though not a professional astronomer I have endeavored [sic] to make myself familiar with the development of astronomical theory and the recent advances that have been made along the lines of physical application and I must say with all due respect to the critics referred to[,] they have failed to show that the major portion of the astronomical facts you cite are in error or that your application of them, in your general argument, is seriously at falt [sic]. Though they have succeeded in pointing out one or two minor errors — (such as proportional to the distance instead of the square of the distance) each of the critic’s [sic] articles have contained errors [sic] serious errors which as professional astronomers they should not have made. Pickering treats the argument more fairly than any of the others and still, in opposition to statement that dark patches such as the "coal sacks" in the Southern portion of the "Milky Way" are actual holes therein he says they may may [sic] really be dark nebula [sic] between us and the Milk[y] Way. When the records of his own observatory will show that these regions to show multitudes of stars on the photographic plate and the analysis of this spectrum shows these stars to be of the same physical structure as the characteristic stars of the Milky Way in the immediate vicinity [2]8 also that they fail to show any extra absorption effects that should show if the light emenating [sic] from them passed through a dark nebula[.] Professor Turner seems to be positive that the nebula photographed around "Nova Persei"9 is a formerly dark nebula illuminat illuminated by light from the nova. Now I have before me a letter from Prof[essor] Perrine10 of the Lick Observatory11 dated May the 10th 1903 in which he expresses doubt of the correctness of this view and while he thinks the question an open one he is inclined to think that the nebula is or was self luminous for several reasons. 1st points of condensation (shown on plates I inclose [sic] you) preserve their formation through moving outwards and longitudinally for great distances — note the amount of these displacements on the plotted plates each square of which represents 2’ of arc (though these plates were taken by Ritchey12 of Yerke’s13 the[y] are the same in effect as Perrine[’]s taken at the Lick)[.] 2nd the light from the nebula failed to show polarization — which it should have shown if reflected at the observed angle. The greatest difficulty he remarks in the way of supposing the light to terminate directly is not the great radial velocity of expansion of [the] nebula but to these account for the great apparent tangential motion — In this instance Prof[essor] Turner shows, to say the least a lack of caution to drag in a doubtful assumption and make it do duty as a certified fact and a fact too illustrating the rapid progress of "astronomical science". Mr Maunder however endeavors [sic] to be the most severe of all as regards ratio of aperture to number of stars[;] he thinks that absorption of the glass "to account in part at least" for the disappearance of the extra stars — failing to note that the reflector was used when determining this point, as well as the refractor[,] and further that Gill14 used a large telescope at the Cape15 when determining this and cut the aperture gradually down but did not thin or thicken the glass. He fails also to observe that the absorption of the ether, cosmic dust, and dark bodies in space were considered by Sir John Herschel16 who thought these considerations insufficient in his "Outlines of Astronomy"17 years ago and further, physisist [sic] though they have sought for it diligently have failed to find any evidence that the "ether" is capable of absorbing heat or light or any other form of energy[,] and even if [3]18 it did absorb[,] an increase of aperture should increase the light grasp[,] otherwise if the universe of ether should if absorbing for an infinite time be now infinitely hot. Mr Maunder’s suggestion that the dark bodies of space are of a "higher order" of impurity than the bright ones, must surely have been put forward as a joke, one would hardly suppose that a number could be found greater than an infinite. Then again the motion of the sun in space coming from the other side of nowhere may be put down to another joke as the exact[?] position of the apex of the sun[’]s way has been shifted, to such an extent as to leave it an open question whether its path is a straight line or a curve[.] Then as to the ability of other planets Galileo19 and the early observational astronomers found it absolutely necessary to explain to everybody that the stars and planets were probably all inhabited [.] The spectroscope as you have observed put the stars themselves beyond the pale and as Pickering remarks there are less than 1% of other stars of the solar type[,] the possible number of planets suitable for life decrease as well — and you go a step further and give reasons for supposing that perhaps the earth alone may be the only inhabited celestial body.

Mr Maunder thinks that the ether[,] if it had a boundary would dissipate into the space beyond — no doubt it would if constituted as a gas, having molecules rebounding against each other but physisists [sic] now insist (namely Kelvin20 for instance) that the ether is a continuous inseparable thing, and if such a medium had boundaries these boundaries would be extremely elastic[,] and any specialized forms of the media rushing [4]21 against the interior surface would be thrown back with the force with which it came — so that it would not need to have come from beyond nowhere nor to go beyond nowhere to keep up its motion even in a straight line[.]

I think sir that you deserve a great deal of thanks for directing attention to points that have been ignored to a great extent by those who are supposed to be specialists in this particular department[.]

Yours very truly | J. R. Collins22 [signature]

(Secretary Royal Ast[ronomical] Soc[iety] of Canada)23

Page numbered 133 in pencil in top RH corner and "J R Collins" written in pencil at the top of the page.
Year deduced from birth and death dates of author.
Wallace, A. R. (1903) Man's Place in the Universe: As Indicated by the New Astronomy Fortnightly Review 73: 395-411.
Pickering, William Henry (1858-1938). American astronomer. He constructed and established several observatories including Percival Lowell’s Flagstaff Observatory. He spent much of the later part of his life at his private observatory in Jamaica.
Maunder, Edward Walter (E. Walter) (1851-1928). British astronomer best known for his study of sunspots and the solar magnetic cycle that led to his identification of the period from 1645 to 1715 now known as the Maunder Minimum.
Turner, Herbert Hall (1861-1930). British astronomer and seismologist. He was Savilian Professor of Astronomy and Director of the Observatory at the University of Oxford 1893-1930.
Flammarion, Nicolas Camille (1842-1925). French astronomer. He was a prolific author, including popular science works about astronomy, several notable early science fiction novels, and works on psychical research.
Page numbered "2" in ink in the centre of top of page.
Nova Persei 1901 (now known as GK Persei), a nova occurring in 1901, was the brightest nova of modern times, until Nova Aquilae in 1918.
Perrine, Charles Dillon (1867-1951). American astronomer living in Argentina. He worked at Lick Observatory (see Endnote 11) from 1893-1909 and accompanied four eclipse expeditions between 1900 and 1908. In 1901, he and George Ritchey (see Endnote 12) observed the apparent superluminal motion in the nebulosity surrounding Nova Persei 1901 (see Endnote 9).
An astronomical observatory constructed between 1876 and 1887, from a bequest from James Lick. It is situated on the summit of Mount Hamilton, east of San Jose, California, USA and owned and operated by the University of California.
Ritchey, George Willis (1864-1945). American optician, telescope maker and astronomer.
An astronomical observatory operated by the University of Chicago in Williams Bay, Winsconsin, founded in 1897 by George Ellery Hale and financed by Charles T. Yerkes. The observatory has the world's largest refracting telescope.
Gill, David (1843-1914). Scottish astronomer, known for measuring astronomical distances, for astrophotography and for geodesy. He spent much of his career at the Royal Observatory at the Cape of Good Hope. He pioneered the use of dry plate photography to create images of the stars. This led to a project in collaboration with the Dutch astronomer J. C. Kapteyn, compiling of an index of brightness and position for some half a million southern stars.
The Royal Observatory at the Cape of Good Hope was founded in 1820, the first scientific institution in Africa, with construction of the main buildings completed in 1829. David Gill (see Endnote 14) was Her Majesty's Astronomer at the Cape of Good Hope from 1879-1906.
Herschel, John Frederick William, 1st Baronet (1792-1871). English polymath, mathematician, astronomer, chemist, inventor and experimental photographer and son of the astronomer William Herschel. He named seven moons of Saturn and four moons of Uranus.
Herschel, J. F. W. (1878) Outlines of Astronomy London, Longmans Green & Co.
Page numbered 134 in pencil in top RH corner. "Royal Astronomical Society of Canada" is printed in top centre of page and "3" written in ink above.
Galileo Galilei (1564-1642). Italian astronomer, physicist, engineer, philosopher and mathematician. He played a major role in the scientific revolution during the Renaissance and is widely considered as one of the greatest scientists of all time. His achievements include improvements to the telescope and consequent astronomical observations.
Thomson, William, 1st Baron Kelvin (1824-1907). British mathematical physicist and engineer. At the University of Glasgow he did important work in the mathematical analysis of electricity and formulation of the first and second laws of thermodynamics. He is widely known for determining the correct value of absolute zero temperature.
Page numbered "4" in ink in the centre of top of page.
British Museum stamp underneath.
Founded in 1868, The Royal Astronomical Society of Canada is Canada's leading astronomy organization.

Please cite as “WCP2826,” in Beccaloni, G. W. (ed.), Ɛpsilon: The Alfred Russel Wallace Collection accessed on 3 May 2024, https://epsilon.ac.uk/view/wallace/letters/WCP2826