Astronomy & Cosmology

First edition, the corrected second printing of this landmark popular work on the quest for the Grand Unified Theory. From the library of physicist Peter Landsberg, with his ownership signature, notes and highlighting, and letter to him loosely inserted.

Peter Landsberg (1922-2010), was a German Jewish refugee to Britain who earned his PhD in quantum mechanics at Imperial College London in 1949 and joined the faculties of the Universities of Cardiff and Southampton. “Landsberg was not solely interested in one branch of physics, he was interested in physics in general and this boyish enthusiasm took his research to all areas of theoretical work”, among them the quantum phenomenon known as bose condensation, the relationship between quantum mechanics and living things, thermodynamics, cosmology, and applications of solar energy. He is best known for his explication of “Landsberg efficiency”, the theoretical limits on how much solar power can be converted to electricity in a given situation (obituary in The Scotsman, May 23, 2010).

Landsberg has made numerous short notes — often page number references — and underlined a number of passages, primarily in chapters 8: The Origin and Fate of the Universe and 9: The Arrow of Time, that deal with thermodynamics and the inflationary model of the universe. Loosely inserted is a typed letter signed to Landsberg from Canon Robert Winnett (1910-1989), to whom the book had been loaned, and who writes that it conveyed to him “a sense of the infinite mystery of the universe, and of unplumbed depths still to be explored, an attitude which is surely akin to the religious”. He goes on the discuss how scientific ideas about the origin of the universe might align with Christianity and other religions, ending with the thought that “we are dealing with probabilities rather than certainties... The origins of religion lie in dimensions of human experience other than the scientific, and any cosmological theory can be interpreted theistically, or if we will, atheistically”.

First edition of this biographical work on the astronomers William, Caroline, and John Herschel by one of the “great popularisers of science of the Victorian period” (Ogilvie, Biographical Dictionary of Women in Science, p. 270). Copies of The Herschels and Modern Astronomy are uncommon on the market, particularly in such a nice example of the publisher’s binding.

Agnes Mary Clerke was taught at home by her scholarly parents, and “by the age of eleven she had mastered Herschel’s Outlines of Astronomy” (Ogilvie, p. 270). Settling in London in 1877, she pursued a career as a writer, producing a remarkable body of work. Clerke “possessed the rare ability to communicate clearly the complexities of scientific theory to a popular audience, while synthesising masses of astronomical information into a coherent whole for professional scientists, who had become so specialised that they could not see the larger connection between their work and other current discoveries in astronomy” (Ogilvie p. 270). Though she never held a position at a university or observatory, Clerke gained “partial admission” to the male-dominated word of astronomy. She had an extensive correspondence with other astronomers, was awarded the Actonian Prize by the Royal Institution, and in 1903 was elected an honorary member of the Royal Astronomical Society.

An interesting archive of unpublished correspondence between leading radio astronomer Alfred Lovell (1913-2012) and astronomer and science populariser Arthur Beer.

Beer (1900-1980) was born in Richenberg, Bohemia (later Czechoslovakia), and educated in Austria and Germany. He worked as an astronomer at Breslau University, where he studied binary stars, and at the German Maritime Observatory. He also wrote newspaper columns and was responsible for developing one of the first scientific radio programmes, Aus Natur und Technik. Beer escaped from Germany in 1934, assisted by Einstein, who wrote him a public letter of recommendation, and spent the rest of his life in the UK. He worked at the Cambridge Solar Physics Observatory and at the Kew Observatory, and became a member of the Royal Astronomical Society. Beer’s most significant contribution to science was as the founding editor of Vistas in Astronomy, a “voluminous and thorough survey of present-day astronomy” in two volumes, conceived as a Festschrift celebrating the 70th birthday of astrophysicist Frederick J. M. Stratton, under whom he had served in Cambridge. The resulting volumes were so impressive that it was continued first as an annual book and then a quarterly journal.

Beer’s correspondent, the astronomer Alfred Lovell, became interested in radar astronomy while working on British military radar projects during the Second World War and seeing unexplained atmospheric phenomena on radar displays. After the war he set up the first radio telescopes at the University of Manchester, establishing his base at Jodrell Bank in Cheshire. His first major success was in using decommissioned military equipment to determine that the radar echoes he’d seen during the war were caused by meteors. In 1950 he convinced the university to fund a large, custom-designed radar telescope, the Mark I, which was finished just in time to track Sputnik and its launch rocket in 1957. “The technical achievement was acclaimed as a national triumph with defence significance–the rocket was essentially an intercontinental ballistic missile, and no other radar system in the world could detect it. The telescope became a national icon, as well as an emblem of the University of Manchester” (ODNB). He continued his work with telescopes Mark 2 and 3, making observations of a variety of astronomical events and bodies, including US and Soviet lunar probes, and later served as a government administrator for large telescope projects. His work was recognised with the award of the royal medal of the Royal Society in 1960, a knighted the following year, and the gold medal of the Royal Astronomical Society in 1981.

This file contains correspondence between Beer and Lovell from the initial conception of the Vistas project in early 1952 through the final stages of printing in December, 1954. Lovell opens with a formal request for papers on February 27th, 1952, and Lovell responds on March 7th, “Thank you for your letter... conveying the invitation to contribute to Professor Stratton’s commemoration volume. I shall be very glad to help with this. It is rather difficult to make suggestions about the nature of the contribution until I know what other radio astronomers might be contributing. For example, the nature of any contributions from the Radio School in Cambridge would obviously influence my own contribution great deal. My provisional answer is, therefore, that I will write about radio astronomy, the exact aspect depending upon what other contributions in this field you are expecting to get. Perhaps you will let me know about this in due course.”

On Mach 5th Beer writes that, “The arrangement of the book has made very good progress in the meantime, and you will be pleased to hear that all essential fields appear to be covered by their leading experts. The main sections will be: - Astronomical Vistas, Dynamical Astronomy... Each section has a number of contributors fro various countries; our latest acquisition was the director of the Mount Wilson and Palomar Observatories... At present the negotiations with publishers are my main preoccupation. For this purpose I am now preparing a provisional list of contributors and suggested titles... Apart from yourself I have only approached two others from your field, namely Ratcliffe and Ryle... Ryle wanted to communicate with you directly as to the question of how to share the radio-astronomical heavens. If you would care to state which part you would like to take over, I shall be delighted to make the necessary arrangements.” Later, in November, he writes to say that he can include a second article by Lovell and wonders if this might also include a drawing or plan of the proposed Mark I telescope. On December 5th Lovell responds, “Thank you for your letter of November 29th, which we discussed when I met you on Wednesday. Subsequently I was able to talk to Ryle and the position now seems quite clear. I shall do my best to let you have two articles from Jodrell Bank - one on Meteors and the other on Pencil Beam Techniques in radio Astronomy, including the new Radio Telescope.”

Additional correspondence follows, primarily related to the forwarding of the articles and illustrations, proofing, and progress with the publishers, with one notable letter from Lovell reading, “I must say that the method used by Pergamon press is excessively irritating and I have never in the whole of my experience had to waste so much time owing to the fact that the proofs and the diagrams have come in bits and pieces over periods of many months. You must be having an awful job on this!”

The two pieces submitted by Lovell were “Large Radio Telescopes and Their Use in Radio Astronomy” (co-authord by R. Hanbury Brown) and “Radio Echo Studies of Meteors” (with J. G. Davies). Of the 16 typed letters signed by Lovell, one has had the signature clipped out to be reproduced in Vistas, and also included in the file is a short autograph note from Lovell’s collaborator R. Hanbury Brown providing a signature as well. There is also a further typed note by Lovell indicating that he wants to approach Lovell for a piece on tracking Sputnik, presumably for a later issue of Vistas, but there is no related correspondence.

First edition, first printing and a beautiful copy inscribed by the author on the title, “Best wishes to my longtime good friend Sy Coleman! John Mather”. The recipient may have been the Sy Coleman who founded Aspen Public Radio and died in 2020.

John C. Mather (1946 - ) is one of the most prominent astrophysicists working today. He was the recipient of the Noble Prize alongside George F. Smoot for their joint work on the cosmic background radiation using data from the COBE satellite, launched in 1989. This groundbreaking research on the energy patterns of the early universe “provided increased support for the Big Bang scenario for the origin of the Universe, as this is the only scenario that predicts the kind of cosmic microwave background radiation measured by COBE. These measurements also marked the inception of cosmology as a precise science” (Nobel Prize announcement).

The Very First Light is Smoot’s first-hand account of the COBE programme and its results, written for a popular audience. Today Smoot is the Senior Project Scientist for the newly launched James Webb Space Telescope, which can see further and in greater detail than any telescope before, promising to revolutionise the field of cosmology.

A rare and evocative lithograph of the Great Comet of 1843 as seen from the Cape of Good Hope, observed and, most unusually, also lithographed by the Astronomer Royal for Scotland, Charles Piazzi Smyth (1819-1900). Copies of this print are exceptionally scarce, with none recorded in COPAC, WorldCat, or auction records. Given that the paper was never published, it seems unlikely that more than a handful were produced.

Smyth was born to well-connected British parents in Naples, his father being a naval officer and respected amateur astronomer, and his mother the daughter of the British Consul to the kingdom of the Two Sicilies. Smyth’s godfather was the famous Sicilian astronomer Giuseppe Piazzi, from whom he received his middle name. Thanks to his father’s connections, at age sixteen Smyth was made assistant to Thomas Maclear, HM Astronomer at the Royal Observatory, Cape of Good Hope. “He spent ten years in southern Africa working in positional astronomy and in arduous geodetic surveys of the province. Encouraged by John Herschel, he experimented in early photography and in 1843 succeeded in producing the oldest known calotypes of people and scenes in southern Africa” (ODNB).

During Smyth’s time in the Cape a remarkable comet appeared in the skies. “The Great March Comet of 1843 was so bright that it was seen in the daytime sky by many people on every continent”, though its brightest and largest appearance was in the southern hemisphere (Stoyan, Atlas of Great Comets). Its tail, measuring up to 70° (more than 350 million kilometers in length), still holds the record for length, and John Herschel described it in 1849 as “by far the most remarkable comet of the century” (Stoyan).

Smyth was a talented amateur artist who frequently painted and sketched, both in connection with his astronomical work and as an observer of the people and landscapes around him. “The naturalistic representations and watercolours by Chales Piazzi Smyth, who was working at the Cape of Good Hope when the comet appeared, are the most impressive reproductions of this apparition of a comet” (Stoyan). Smyth was particularly interested in printing techniques and their applications to scientific illustration. His first major published work was a paper submitted to the Royal Astronomical Society on this subject, in which he “reviews critically the illustrations in several recent publications and discourses with apparent authority on the processes of engraving, aquatintintg and mezzotinting. He suggests modifications that might be used to yield more subtle effects” (Warner, Charles Pizaai Smyth: Astronomer-Artist, His Cape Years, p. 113).

Smyth’s proficiency with lithography and copperplate engraving allowed him to print the illustrations for his own papers, a practice that was (and indeed, still is) unusual (Warner, p. 113). In 1846 he was appointed Astronomer Royal at Edinburgh, “the hub of the printing and illustration industry... in these circumstances he did not need to acquire a press, but bought or hired stones on which he could draw his pictures and then send the stones to the nearest printer. Piazzi was engaged in lithographing of his sketches ‘The Zodiacal Light as Seen at the Cape of Good Hope’ and ‘The Great Comet of 1843’ —to be used in his published accounts— when [his friend from South Africa, the artist] Charles Bell arrived in 1847”. At first, Piazzi sent his stones to the printer W. Walton, who was probably responsible for this print, but later Bell purchased a press which he and Piazzi shared (Warner, pp. 114-115).

Both The Great Comet and The Zodiacal Light were meant to illustrate Smyth’s unpublished paper “Attempt to apply instrumental measurement to the zodiacal light”, which was completed on March 25th, 1848, received by the Royal Society on the 13th of April, and withdrawn on the 2nd of November. The manuscript and the original painting are still at the Royal Society and have been digitised (references AP/30/18 and AP/30/18/5), and two oil paintings of the comet by Smyth are held at the National Maritime Museum at Greenwich (object ID BHC4148 and BHC4147). This copy of the lithograph is especially intriguing because of the pencilled annotation where Smith’s printed initials should be: “CPS del[iniavit] & lit”, indicating that he made the lithograph himself. Though the writing is dissimilar to Smyth’s formal hand, the likeliest explanation is that it was inserted by himself or someone close to him.

A rare and evocative lithograph of the zodiacal light as seen from the Breede River in South Africa, observed and, most unusually, lithographed by the Astronomer Royal for Scotland, Charles Piazzi Smyth (1819-1900). Smyth’s print was “the first attempt to furnish a realistic depiction of this elusive feature” of the night sky (Warner, Charles Pizaai Smyth: Astronomer-Artist, His Cape Years, p. 101). Copies of this lithograph are exceptionally scarce. We can locate only one, in the Herschel family collection at the National Maritime Museum in Greenwich (object ID PAH6023). Searches of COPAC, WorldCat, and auction records trace no others. Given that the paper they were designed to illustrate was never published, it seems unlikely that more than a handful were ever produced.

Smyth was born to well-connected British parents in Naples, his father being a naval officer and respected amateur astronomer, and his mother the daughter of the British Consul to the kingdom of the Two Sicilies. Smyth’s godfather was the famous Sicilian astronomer Giuseppe Piazzi, from whom he received his middle name. Thanks to his father’s connections, at age sixteen Smyth was made assistant to Thomas Maclear, HM Astronomer at the Royal Observatory, Cape of Good Hope. “He spent ten years in southern Africa working in positional astronomy and in arduous geodetic surveys of the province. Encouraged by John Herschel, he experimented in early photography and in 1843 succeeded in producing the oldest known calotypes of people and scenes in southern Africa” (ODNB). It was during this period that Smyth attempted observations of the zodiacal light. This is the glow, also known as the false dawn, which appears along the ecliptic at twilight and just before sunrise, and is caused by light from the sun reflecting off interplanetary dust.

In addition to photography, Smyth was a talented amateur artist who frequently painted and sketched, both in connection with his astronomical work and as an observer of the people and landscapes around him. His depictions of the Great Comet of 1843 are now considered “the most impressive” illustrations of that apparition (Stoyan, Atlas of Great Comets). Smyth was particularly interested in printing techniques and their applications to scientific illustration. His first major published work was a paper submitted to the Royal Astronomical Society on this subject, in which he “reviews critically the illustrations in several recent publications and discourses with apparent authority on the processes of engraving, aquatintintg and mezzotinting. He suggests modifications that might be used to yield more subtle effects” (Warner, p. 113).

Smyth’s proficiency with lithography and copperplate engraving allowed him to print the illustrations for his own papers, a practice that was (and indeed, still is) unusual (Warner, p. 113). In 1846 he was appointed Astronomer Royal at Edinburgh, “the hub of the printing and illustration industry... in these circumstances he did not need to acquire a press, but bought or hired stones on which he could draw his pictures and then send the stones to the nearest printer. Piazzi was engaged in lithographing of his sketches ‘The Zodiacal Light as Seen at the Cape of Good Hope’ and ‘The Great Comet of 1843’ —to be used in his published accounts— when [his friend from South Africa, the artist] Charles Bell arrived in 1847”. At first, Piazzi sent his stones to the printer W. Walton, who was probably responsible for this print, but later Bell purchased a press which he and Piazzi shared (Warner, pp. 114-115).

Both The Zodiacial Light and Great Comet were meant to illustrate Smyth’s unpublished paper “Attempt to apply instrumental measurement to the zodiacal light”, which was completed on March 25th, 1848, received by the Royal Society on the 13th of April, and withdrawn on the 2nd of November. The manuscript and the original painting are still at the Royal Society and have been digitised (references AP/30/18 and AP/30/18/7). This copy of the lithograph is especially intriguing because of the pencilled annotation next to Smith’s printed initials, “del[iniavit] & lit”, indicating that Smyth made the lithograph himself. Though the writing is dissimilar to Smyth’s formal hand, the likeliest explanation is that it was inserted by himself or someone close to him. This annotation does not appear in the NMM copy.

The zodiacal light continued to be an interest of Smyth’s throughout his career, particularly in the 1870s when he turned his attention to “spectroscopy and the ‘new astronomy’, a term used to denote the area of astronomy later known as astrophysics... One of his aims, successfully carried out, was to discriminate in the sun's spectrum between absorption lines of purely solar origin and those produced in the earth's atmosphere. Among other researches were studies of the spectra of the aurora (observed from Edinburgh), the zodiacal light (observed from Palermo), and the so-called rainband, due to atmospheric water vapour. In the laboratory he concentrated on the spectra of diatomic molecules and, in collaboration with Alexander Stewart Herschel, deciphered the harmonic structure of the green carbon monoxide band” (ODNB).

Sixth printing, published in the same year as the first. Presentation copy inscribed by the author in elaborate calligraphy on the half title, “To: Ravonne, Welcome to the Universe, Neil D. Tyson, May 2007”. Uncommon signed. The present volume is a collection of forty-two essays originally published in Tyson’s “Universe” column in Natural History Magazine between 1995 and 2005.

Astrophysicist Neil DeGrasse Tyson’s (1958 - ) interest in astronomy began during childhood, when he viewed the Moon’s surface through a friend’s binoculars. Tyson studied at Harvard, the University of Texas, and Columbia, then joined the faculty of Princeton, where “many students found him a particularly inspiring professor” (Krapp, Notable Black American Scientists, p. 304). His academic research has been focused on cosmology, particularly star births and supernovae, and the structure of the Milky Way and other galaxies.

Throughout his career Tyson has also been focused on sharing astronomy with the general public, leading to him becoming one of the world’s most famous scientists. Since 1996 he has been the director of the Hayden Planetarium in New York; written columns in popular magazines; published sixteen books; become a popular figure on Twitter; and hosted several television shows, including the 2004 PBS series Origins and the 2014 reboot of Carl Sagan’s Cosmos. His reputation, however, has been affected by rape and sexual harassment allegations made public by fellow graduate student Thchiya Amet El Maat, professor Katelyn Allers, former assistant Ashley Watson, and an anonymous woman in late 2018.

An archive of correspondence between astronomer Arthur Beer and Nobel Prize winning chemist Harold Urey regarding the latter’s contribution to Vistas in Astronomy.

Beer (1900-1980) was born in Richenberg, Bohemia (later Czechoslovakia), and educated in Austria and Germany. He worked as an astronomer at Breslau University, where he studied binary stars, and at the German Maritime Observatory. He also wrote newspaper columns and was responsible for developing one of the first scientific radio programmes, Aus Natur und Technik. Beer escaped from Germany in 1934, assisted by Einstein, who wrote him a public letter of recommendation, and spent the rest of his life in the UK. He worked at the Cambridge Solar Physics Observatory and at the Kew Observatory, and became a member of the Royal Astronomical Society. Beer’s most significant contribution to science was as the founding editor of Vistas in Astronomy, a “voluminous and thorough survey of present-day astronomy” in two volumes, conceived as a Festschrift celebrating the 70th birthday of astrophysicist Frederick J. M. Stratton, under whom he had served in Cambridge. The resulting volumes were so impressive that it was continued first as an annual book and then a quarterly journal.

American chemist Harold Urey (1893-1981) did key work on atomic and molecular structures, particularly hydrogen isotopes. This led him to the discovery of deuterium, for which he was awarded the Nobel Prize in 1934. During the Second World War he led the Manhattan Project’s branch at Columbia University, where he applied his knowledge of isotope separation techniques to the problem of isolating of pure uranium 235 on an industrial scale. After the war he worked at the Institute for Nuclear Studies at the University of Chicago. In 1958 Urey moved to the University of California, San Diego, where he did groundbreaking work on the origins of life on Earth, conducting a laboratory simulation of the conditions on the early Earth and proving that they were ideal for the production of cellular building blocks such as amino acids.

The correspondence present here consists of five letters from Urey, mainly on practical issues connected with his contribution to Beer’s book. In the first, on September 10th, 1952, he replies to Beer’s request for submissions, apologising for taking so long to reply as “I have not been able to think of a subkect to write about. I am leaving for Europe on the 14th of September and hope to visit Cambridge about October 15th. If it isn’t too late by that time perhaps we can discuss the question then. In the meantime, I will turn this over in my mind and try to think of something that I might contribute to the book.” On January 8th the following year he writes, “At last the paper for the Stratton volume!... I wish it were a better paper. If you do not wish to publish it I shall not be offended at all. There are quite a few notes and I believe references and notes are more easily read if placed at the bottom of the page. But perhaps your rules are all made long ago.” Later that month Urey sends short note to confirm receipt of the document, and in July he asks that the proofs be mailed to him in Stockholm. The final letter, dated by Beer in pencil as postmarked July 31st, 1953, discusses the terms he has chosen for the index (”I have underlined [in the returned proof, not present here] expressions indicating topics for the index... on the margins I have written additional suggestions” and relates that the illustrations had not arrived yet when he left for the states, but that “I believe the figures can be assumed to be all right”.

James E. Webb (1906-1996) was NASA’s second administrator and one of its most significant, seeing the agency through the Mercury and Gemini programs and the preparation for the Apollo missions.

To Webb, “the space program was more than a political race. He believed that NASA had to strike a balance between human space flight and science because such a combination would serve as a catalyst for strengthening the nation's universities and aerospace industry... Webb's vision of a balanced program resulted in a decade of space science research that remains unparalleled today. During his tenure, NASA invested in the development of robotic spacecraft, which explored the lunar environment so that astronauts could do so later, and it sent scientific probes to Mars and Venus, giving Americans their first-ever view of the strange landscape of outer space. As early as 1965, Webb also had written that a major space telescope, then known as the Large Space Telescope, should become a major NASA effort. By the time Webb retired just a few months before the first moon landing in July 1969, NASA had launched more than 75 space science missions to study the stars and galaxies, our own Sun and the as-yet unknown environment of space above the Earth's atmosphere. Missions such as the Orbiting Solar Observatory and the Explorer series of astronomical satellites built the foundation for the most successful period of astronomical discovery in history, which continues today”. Webb also “enhanced the role of scientists in key ways. He gave them greater control in the selection process of science missions and he created the NASA University Program, which established grants for space research, funded the construction of new laboratories at universities and provided fellowships for graduate students” (”Who is James Webb?”, NASA James Webb Space Telescope website).

Webb’s legacy has been complicated by allegations that at the State Department and NASA he played a leading role in the lavender scare, in which hundreds of gay personnel were fired from the federal government. In 2021 four astronomers published an op-ed in Scientific American requesting the renaming of the soon-to-be-launched James Webb Space Telescope, but NASA administrators announced that an inquiry into Webb’s actions determined it was unlikely he had played a key role in the firings and the name would be kept.

These pamphlets deal with various aspects of space science and the space race. “Man Must Take Environment into Space” discusses the hostile environment of space and the ways that NASA scientists have prepared their vehicles and crew for it. “Administration and Management of Space Exploration” lays out the structure and goals of NASA, and “From Runnymede to Ganymede” is the text of a historical talk that Webb gave at the Celebration of the Prelude to Independence in Williamsburg, Virginia on May 27th, 1967.

A dramatic and uncommon mezzotint depicting the spectacular meteor seen in London on February 11th, 1850, by the prominent court artist Matthew Coates Wyatt (1777-1862). One other copy of this print appears in recent auction records, sold at Galerie Bassenge in 2016, and institutional copies are held at the National Maritime Museum at Greenwich, Museum Bojmans in Rotterdam, the Museum of Fine Arts Boston, and the British Museum, which has George Cruikshank’s copy, presented to him by the artist.

“In 1850 a huge meteor appeared over England and was visible in London. It was captured dramatically by Matthew Coates Wyatt over Paddington in a mezzotint that suggests, due to the explosion and sparks of its head, that it was a bolide... Other accounts and representations from various locations were reported in the Illustrated London News... as well as in other periodicals. James Glaisher, the assistant to the Astronomer Royal, published an appeal for additional reports in the same issue, and consequently so many accounts were sent in that Glaisher had them published in the Philosophical Magazine” (Olson & Pasachoff, Fire in the Sky: Comets and Meteors, the Decisive Centuries in British Art and Science, pp. 213-214).

“By good luck, the painter and sculptor Matthew Cotes Wyatt happened to witness the meteor over Paddington; sensing a market, he published this velvety mezzotint of the view two months later... The technique had largely gone out of fashion by 1850, but the rich darks and brilliant lights that it allows were a perfect choice for this dramatic nighttime scene” (Museum of Fine Arts Boston).

Wyatt was the youngest son of the architect James Wyatt and a favourite in the court of George III. “His designs represented a dramatic and full-blooded union of neo-classicism and baroque revival. He was more a theatrical designer than a sculptor in the conventional sense” (ODNB). Wyatt was responsible for a number of significant commissions, including the ceiling of the concert room at Hanover Square; the Nelson monument in the Exchange Flags at Liverpool; Princess Charlotte’s marble cenotaph in St. George’s Chapel at Windsor; the bronze equestrian statue of George III that stands in Pall Mall East; and extensive decorative work at Belvoir Castle, home of the Duke of Rutland.