Appendix H
In Troilus and Cressida, Ulysses places Earth at the centre of the heavens but gives the Sun the authority of a king. This combination invites a reading alongside the astronomical problem Henry Savile investigated during his travels with Neville: how could Copernicus’s account of planetary motion be used without accepting Earth’s annual revolution around the Sun? Savile’s surviving diagrams and letters document his work on that question in 1581. Dudith then wrote directly to Neville asking him to press Savile for an explanation of Copernicus. The connection begins with an identifiable intellectual problem, pursued by Neville’s tutor and discussed in a letter addressed to Neville himself.1
Ulysses’s planetary order
The Greek commanders are discussing why their army has failed. Ulysses blames the neglect of rank and authority, turning to the heavens for his governing analogy:
The heavens themselves, the planets, and this center
Observe degree, priority, and place,
Insisture, course, proportion, season, form,
Office, and custom, in all line of order.
And therefore is the glorious planet Sol
In noble eminence enthroned and sphered
Amidst the other, whose med’cinable eye
Corrects the influence of evil planets,
And posts, like the commandment of a king,
Sans check, to good and bad. But when the planets
In evil mixture to disorder wander,
What plagues and what portents, what mutiny,
What raging of the sea, shaking of Earth,
Commotion in the winds, frights, changes, horrors
Divert and crack, rend and deracinate
The unity and married calm of states
Quite from their fixture! […]— Troilus and Cressida, 1.3, Ulysses.2
The speech separates position from power. Earth is “this center,” but the commanding body is “planet Sol,” enthroned among its fellows. Its influence reaches good and bad alike, without obstruction, like a king’s command. Ulysses needs both an ordered place for every body and an authority capable of governing the whole. The Sun supplies that authority.
Thomas Digges gives the comparison a sharper focus. In his Perfit Description, which sets out a Copernican universe, he describes the Sun:
like a king in the middest of all reigneth and giveth laws of motion to the rest.3
Digges joins central position and royal power in the Sun. Ulysses distributes them: Earth is “this center,” while the Sun is enthroned “amidst the other” and exercises the “commandment of a king.” Digges describes the government of celestial motion; Ulysses turns celestial government into an argument about political order. Their shared image of solar kingship makes the difference in the Sun’s position especially interesting.4
Savile’s investigations give this comparison a concrete setting within Neville’s life. Copernicus’s mathematical account of the planets could be studied and adapted without accepting his placement of Earth in motion around the Sun. This was precisely the problem Savile pursued with Wittich during the European journey. The reading proposed here places Ulysses’s combination of terrestrial centrality and solar authority alongside that documented inquiry.5
Savile, Wittich and Neville
In 1581 Henry Savile was studying with Paul Wittich at Breslau, where Andreas Dudith maintained a household that welcomed scholars and supported mathematical inquiry. Wittich had spent several months with Tycho at Uraniborg in 1580. Neville’s travels with Savile thus brought him into a scholarly circle whose work connected directly with the astronomical investigations taking place at Tycho’s observatory.1
Savile’s surviving papers show the investigation taking shape. In a draft letter to the astronomer Johannes Praetorius, he proposed a central Earth that still rotated daily on its axis and asked how the planetary circles could be arranged to agree with Copernicus’s calculations. He began by asserting a result, then changed dico (“I say”) to quaero an (“I ask whether”). In later notes and correspondence he recorded five alternative arrangements for the superior planets—Mars, Jupiter and Saturn—discussed with Wittich. Different arrangements could reproduce the same observed motions. His notes and diagrams survive in two Bodleian manuscripts, Savile 47 and Savile 108.6
Savile also prepared an explanation of Copernicus’s account of Earth’s threefold motion for Dudith, dated 22 March 1581. Dudith’s interest was sustained: he wanted someone able to make the difficult mathematics intelligible.7
Neville himself appears in this correspondence. On 7 August 1581, when Neville and Savile were in Venice, Dudith wrote to Neville asking him to spur Savile to further work:
Urge Savile, I beg you, most earnestly, and press him harder to prepare something for me on the obscure passages of the ancient mathematicians, and on Copernicus, who should be compared with the ancients—or, if Wittich is to be believed, preferred to them.
Dudith’s Latin poses the choice: comparandum aut, si credendum est Wittichio, anteponendum. The question was whether Copernicus should be set beside the ancient authorities or placed above them. In the same letter Dudith asked what Neville wanted done with the books he had left behind and requested further mathematical and philosophical works. Neville was being asked to help obtain both texts and explanations.8
Dudith’s request drew Neville personally into a continuing exchange about the old and new astronomy. Savile’s investigations belonged to 1581, seven years before Tycho published his completed system.9
Tycho’s solution
Tycho Brahe (1546–1601), a Danish nobleman and astronomer, established Uraniborg on the island of Hven in 1576 with royal support. Working before astronomical telescopes, he built a programme of precise observation using large sighting instruments.10 His measurements placed the new star of 1572 and the comet of 1577 beyond the Moon, challenging the idea of unchanging heavens and, in the comet’s case, solid planetary shells.11
In 1588 he published his alternative to Copernicus in De mundi aetherei recentioribus phaenomenis: Earth remained stationary, but the five other planets travelled around the Sun, which itself travelled around Earth. The principal arrangements were:
| System | Earth | Sun and other planets |
|---|---|---|
| Ptolemaic | Stationary at the centre | Sun, Moon and planets move around Earth. |
| Copernican | Rotates and travels around the Sun | The planets, including Earth, travel around the Sun; the Moon travels around Earth. |
| Tychonic | Stationary at the centre | Sun and Moon travel around Earth; Mercury, Venus, Mars, Jupiter and Saturn travel around the Sun. |
Tycho thus gave the Sun an organising role within an Earth-centred universe. His observations also outlasted his own model: Kepler used them to establish the motions of the planets.12
Tycho’s books in the Savile circle
The later correspondence supplies a second connection. Henry Savile’s younger brother Thomas undertook his own European tour in 1588–1591, visiting Dudith and subsequently working with Gian Vincenzo Pinelli in Padua. Like Henry, Thomas combined Greek scholarship with mathematics and astronomy; while at Breslau he completed a Latin translation of the ancient astronomical writer Geminus.13
On 20 November 1588 Dudith asked Johannes Praetorius about Tycho’s newly printed book and expressed his wish to inscribe a globe with stars positioned from Tycho’s observations, which he considered more accurate than others. On 11 December he asked Tadeáš Hájek to thank Tycho for his gift, promising to write after studying the whole book. Thomas Savile was then with Dudith and sent greetings in the same letter.14
Dudith was still seeking Henry’s earlier work. On 14 January 1589, after Thomas’s arrival and the receipt of Tycho’s book, he asked Praetorius to return Henry Savile’s explanation of Earth’s threefold motion, adding a clear diagram and any necessary annotations. The explanation prepared in 1581 remained part of the household’s astronomical discussions eight years later.7
Eleven days later, on 25 January 1589, Dudith described a diagram associated with Wittich which resembled Tycho’s new hypotheses and asked Praetorius to examine both. This was the same household in which Henry Savile had worked years earlier, now receiving and discussing Tycho’s published astronomy while Thomas Savile was present.15
Tycho’s own letter to Thomas Savile, dated 1 December 1590, is still more explicit. Thomas had written to him from Hamburg and had intended to visit Hven, but adverse winds and seas had prevented the journey. He had also requested Tycho’s book eagerly. Tycho responded by sending two copies of his second book on recent celestial phenomena and asked Thomas to show it to John Dee and Thomas Digges so that they could examine it and give their opinions freely. Astronomy travelled through this circle as books to be read, criticised and discussed. Tycho also sought literary recognition. His postscript begins:
Addidi quaterna Exemplaria meæ Effigiei nuper Amsterodami cupro insculptæ.
I have added four copies of my portrait, recently engraved in copper at Amsterdam.
He then asked whether excellent English poets might compose an epigram on the portrait and in praise of his work, mentioning Daniel Rogers as a possible contributor. The request deliberately joined the circulation of astronomy to the circulation of poetry.16
Thomas also forwarded Italian newsletters to Neville. Sixteen newsletters addressed to Thomas Savell of London in 1591 survive among Neville’s diplomatic papers, carrying reports from Rome and Venice. Discussed in the Othello chapter, they give a concrete example of Thomas passing continental information to Neville: the recipient of Tycho’s books and portraits was also a supplier of Neville’s news.17
Rosencrantz, Guildenstern and Hamlet
Jacques de Gheyn’s engraved portrait of Tycho surrounds him with the arms and names of his ancestors. Among them are “ROSENKRANS,” on the left side of the arch, and “GVLDENSTEREN,” near the foot of the left column. The conjunction of the two names has long attracted attention in discussions of Hamlet.18 The portrait and Thomas Savile’s connection with its circulation are already described in the Hamlet chapter.19
The correspondence gives this comparison a particular interest for Neville. The intended recipient of the portraits was his tutor’s brother, and Tycho expressly wanted them brought to the attention of English poets. The same letter directed Thomas towards Digges and Dee. Here the names in Shakespeare’s Danish tragedy occur on an object that Tycho was sending into an identifiable English scholarly and literary circle.16
Hamlet’s own astronomical language appears in his letter to Ophelia:
Doubt thou the stars are fire,
Doubt that the sun doth move,
Doubt truth to be a liar,
But never doubt I love.
Copernicans did question whether the Sun moved; both Ptolemy and Tycho retained a moving Sun. Later Hamlet says he could be confined in a nutshell and count himself a “king of infinite space.” That passage survives in the First Folio but is absent from the Second Quarto. Whether these lines invoke a particular astronomer or draw on a broader debate, the movements of the Sun and the extent of the heavens offered Shakespeare material for thinking about certainty, confinement and freedom.20
The comparison begins with words on the page: Digges’s Sun reigns from the centre; Ulysses names Earth as the centre and gives the Sun command. Behind it lies a documented question pursued within Neville’s circle—how to reconcile the old celestial order with the new planetary mathematics. Savile’s papers record the inquiry, Dudith’s letter brings Neville into it, and Thomas Savile’s correspondence continues the exchange through Tycho’s books and portraits.
Notes and sources
Robert Goulding, “Henry Savile and the Tychonic World-System”, Journal of the Warburg and Courtauld Institutes 58 (1995), 152–179, especially 163–175. His evidence includes Oxford, Bodleian Library, MSS Savile 47 and Savile 108. Manuscript readings and identifications here follow his published study. Wittich’s visit to Tycho in 1580 and his subsequent work with Savile establish a personal connection, but do not establish that Savile knew everything Wittich had discussed with Tycho.↩︎
Shakespeare, Troilus and Cressida, 1.3, Folger Shakespeare Library. Lineation retained; emphasis added. The quotation ends before Ulysses’s next sentence.↩︎
Thomas Digges, “To the Reader,” A Perfit Description of the Caelestiall Orbes, appended to Leonard Digges, A Prognostication Everlasting (1596), sig. M1r, digitised edition. Spelling modernised from the printed leaf, retaining “middest,” “reigneth” and “giveth.” The Perfit Description first appeared in 1576; the wording quoted here was checked in the 1596 printing. The correspondence is one of imagery and thought: Digges explicitly affirms Earth’s annual movement, whereas Ulysses’s speech does not.↩︎
The distinction between position and governing authority is the reading developed here. A specifically Tychonic identification remains debatable. Anna Cetera-Włodarczyk, Jonathan Hope and Jarosław Włodarczyk, “Unsphered, Disorbed, Decentred: Shakespeare’s Astronomical Imagination,” Shakespeare 17.4 (2021), 400–427, conclusion and note 71, article, identify “sphered” here as one of Shakespeare’s two explicitly Ptolemaic uses of “sphere,” while arguing more broadly that Shakespeare responded imaginatively to contemporary astronomical debates. The point at issue is whether “amidst” gives the Sun the orbital centrality Moore and Wember infer, or its middle position in the traditional order of seven planets. “Sphered” also raises a question about how literally to read the celestial machinery, since Tycho rejected solid planetary shells. The speech does not explicitly say that the five planets orbit the Sun. Its compatibility with Tycho should therefore be distinguished from a uniquely demonstrated identification. The speech’s silence about solar orbits does not positively identify it with Savile’s experimental models either. Ulysses speaks of the Sun correcting planetary influence, an astrological function; Digges explicitly speaks of laws of motion. The comparison here concerns their treatment of position and authority, not identical physical claims. For the differing approaches to Copernicus taken by Savile and Digges, see Goulding, pp. 153–154.↩︎
Peter R. Moore, “Shakespeare’s Astronomy,” Shakespeare Oxford Society Newsletter 24.3 (Summer 1988), p. 5, original article, PDF p. 34; Hanno Wember, “Illuminating Eclipses: Astronomy and Chronology in King Lear,” Brief Chronicles II (2010), 32–43, especially 34–35 and note 6, article. Moore identifies “this center” with Earth, takes “planet Sol” to retain a moving Sun, and reads solar kingship “amidst the other” as the Sun’s central relation to the planets in Tycho’s system. Wember expressly credits Moore and argues by exclusion: the moving Sun rules out Copernicus, while the Sun’s centrality rules out Ptolemy. These are the prior published Tychonic readings, not independent discoveries claimed here. The present argument draws its historical foundation from Goulding’s reconstruction of Savile’s papers and distinguishes the speech’s distribution of position and authority from a technical description of planetary orbits. Neither Moore’s nor Wember’s identification is assumed as an established result.↩︎
Goulding, “Henry Savile,” pp. 163–165 for the central-Earth proposal retaining daily rotation and axial precession, and the change from dico to quaero an; pp. 167–168 for the diagrams and equivalent constructions; pp. 171–173 for the five models of the superior planets and the draft correspondence. He tentatively places the first draft in January 1581 and the second in March, reconstructing their sequence from the letters mentioned and the development of Savile’s questions. The planetary diagrams in the draft and the separate notes share their identifying Greek and Roman letters. Savile’s surviving conclusion expresses uncertainty about the models’ truth; the manuscript breaks off. Goulding’s discussion of Savile’s mathematical understanding and his role as a recorder of Wittich’s work is at pp. 178–179. The manuscripts themselves have not been independently collated here.↩︎
Goulding, “Henry Savile,” p. 165 n. 48 and p. 167 n. 49. The summary dated 22 March 1581 explained the astronomical function of the three motions Copernicus assigned to Earth. Dudith requested its return on 27 October 1583, 10 January 1584 and 14 January 1589, the last after Thomas Savile’s arrival. In the 1589 request he remembered having sent Praetorius the explanation Henry had prepared for him, could find no copy among his papers, and asked for a copy with a diagram and any annotations Praetorius thought necessary. Goulding cites the surviving letter-book copy at Esztergom, Főszékesegyházi Könyvtár, Cat. V. Tit. IV/d, p. 85. This account follows Goulding’s transcription and discussion, not a fresh inspection of that manuscript.↩︎
Andreas Dudith, Epistulae, VII, 1581–1589 (Budapest, 2019), no. 1072, 7 August 1581, pp. 87–88, critical edition. English translation here from the edition’s Latin. The edition identifies the surviving draft as Berlin, Staatsbibliothek, Depot Breslau, R 253, no. 19, f. 10r. For Neville and Savile in Venice, and the accompanying requests addressed to Savile, see Goulding, p. 175 and n. 78. The published edition, rather than the original manuscript, was checked for this draft.↩︎
Goulding, “Henry Savile,” 175–179, especially pp. 177–178: the notes distinguish experimental heliocentric arrangements from their geocentric equivalents. The models recorded in 1581 did not retain even the Capellan arrangement in which Mercury and Venus orbit the Sun; their adjustments for those planets instead involved additional epicycles. They must not be conflated with Tycho’s later system. Goulding assigns the final development to Tycho while explaining Wittich’s contribution to the underlying mathematics.↩︎
Ronald Brashear, introduction to Tycho Brahe, Astronomiæ instauratæ mechanica (1598), Smithsonian Libraries, digital exhibition; History of Science Museum, Oxford, “Images of Tycho Brahe: Tycho Brahe”.↩︎
High Altitude Observatory, NSF National Center for Atmospheric Research, “Tycho Brahe (1546–1601)”, sections on the 1572 nova and the 1577 comet. For the wider significance of the dissolution of celestial spheres, see Cetera-Włodarczyk, Hope and Włodarczyk, “Unsphered, Disorbed, Decentred,” section “Shakespeare, Ptolemy, Copernicus and Beyond.”↩︎
Robert Goulding, “Henry Savile and the Tychonic World-System”, Journal of the Warburg and Courtauld Institutes 58 (1995), 152–179, especially 152–161. The table gives the basic arrangements, not the full geometrical machinery for calculating motion. For Kepler’s use of Tycho’s observations, see Brashear’s Smithsonian introduction.↩︎
Robert B. Todd, “Henry and Thomas Savile in Italy”, Bibliothèque d’Humanisme et Renaissance 58.2 (1996), 439–444, especially 439 and 442–444. Thomas’s tour was separate from Henry’s earlier journey with Neville; Todd corrects the claim that the brothers travelled together, p. 440 n. 7. Thomas completed his Geminus translation at Breslau on 14 November 1588.↩︎
Dudith, Epistulae, VII, no. 1281, 20 November 1588, pp. 584–588, particularly 586–587; no. 1284, 11 December 1588, pp. 591–592. Note 7 at p. 592 identifies the Savile present as Thomas. Dudith asks that thanks be conveyed to Tycho for his gift and says he will write after reading the whole book: “Scribam ad eum, postquam totum eius librum cognovero.”↩︎
Dudith, Epistulae, VII, no. 1294, 25 January 1589, pp. 616–619, particularly 618–619; Goulding, 176–177. The surviving letter is a later copy and its diagram may simplify the original. It is evidence of discussion and comparison, not a secure reproduction of every detail of Wittich’s model.↩︎
Tycho Brahe to Thomas Savile, 1 December 1590, ed. Peter Zeeberg, Tekstnet; J. L. E. Dreyer, ed., Tychonis Brahe Dani Opera Omnia, VII (Copenhagen, 1924), 283–285. English translation of the postscript’s first sentence supplied here. The edition identifies the manuscript as British Library, Harley MS 6995, item 40. The letter records the sending of books and portraits and the request for epigrams; it does not identify a subsequent poem or establish which individuals viewed a portrait.↩︎
The National Archives, PRO 30/50/70/2, “Sixteen newsletters addressed to Thomas Savell of London by an anonymous correspondent, dated from Rome and Venice; in Italian,” catalogued September–November 1591, item catalogue; PRO 30/50/70, “Additional diplomatic correspondence of Sir Henry Neville,” parent catalogue. The packet documents the newsletter connection; it does not establish that Tycho’s books or portraits accompanied the newsletters.↩︎
Peter Usher develops the portrait connection into a cosmic allegory: Rosencrantz and Guildenstern represent Tycho’s hybrid cosmos, Claudius evokes Claudius Ptolemy, and Hamlet’s “infinite space” evokes the expanded universe associated with Thomas Digges. He also discusses the proposal that the opening scene’s star recalls the nova of 1572, observed by both Tycho and Digges. See “Advances in the Hamlet Cosmic Allegory”, The Oxfordian 4 (2001), 25–49, especially 29–34 and 42–44. At p. 30 he credits Donald W. Olson, Marilynn S. Olson and Russell L. Doescher with the nova identification; that proposal is reported here through Usher. Alan S. Weber, “What Did Shakespeare Know About Copernicanism?”, Romanian Journal of English Studies 9.1 (2012), 351–365, especially 357–362, criticises the more elaborate claims of otherwise unknown telescopic discoveries encoded in the play, while taking more seriously Digges’s possible influence on Shakespeare’s imaginative treatment of infinity. At p. 358 he also discusses the English visit of Frederik Rosenkrantz and Knud Gyldenstierne in 1592 as an alternative explanation for the courtiers’ names. These interpretations are distinct from the documented contents of Tycho’s letter and do not establish Neville’s own cosmological allegiance.↩︎
Jacques de Gheyn II, Tycho Brahe, Statens Museum for Kunst, KKSgb7575, catalogued 1588–1590. The inscription gives Tycho’s age and the year 1586; that is not necessarily the printing date of a particular impression. The shields display ancestral names. For the history of the Hamlet comparison, see Usher, p. 29, and Weber, pp. 357–358, cited in the preceding note. Usher credits the portrait proposal to Leslie Hotson.↩︎
Shakespeare, Hamlet, 2.2, and Folger’s introduction to the text. The Folger lineation is retained in the verse. For the editorial discussion of “Doubt that the sun doth move,” see Weber, pp. 355–357. “Infinite space” is present in the First Folio (1623), absent from Q2 (1604/5); the textual distinction is discussed further in “Hamlet’s Infinite Space,” Appendix G.↩︎