Stars that are not Suns

Johannes Kepler embraced the idea of extraterrestrial intelligent life. He wrote favourably about the possibility of intelligent life on Jupiter, for example, supposing that all its moons surely served the Jovians well, illuminating the skies of that stupendous world (Kepler, Reference Kepler1965: 39–47). But he would have rejected SETI on scientific grounds. He determined that there was but one sun in the universe – ours.

Kepler said in his 1610 Conversation with Galileo's Starry Messenger that the simplest observations, measurements and calculations proved Bruno wrong. ‘To use Bruno's terms, the [fixed stars] are suns’, Kepler wrote, ‘Nevertheless, let him not lead us on to his belief in infinite worlds, as numerous as the fixed stars and all similar to our own’. Noting that Galileo reported over 10 000 telescopically visible stars, Kepler continued (Kepler, Reference Kepler1965: 34–35),

Astronomers from Ptolemy in the 2nd century to Tycho Brahe in the 16th had repeatedly measured the apparent diameters of visible stars to be ~1 arc minute (Van Helden, Reference Van Helden1985: 15–53), unaware that these diameters were optical artefacts and thus did not reflect physical sizes (unlike the apparent diameters of the sun and moon). Kepler continues:

In other words, Kepler argued that stars are too dim to be bodies like our sun. Their light is infinitely weaker, practically speaking, despite their combined apparent size rivalling the sun. And since astronomers understood the stars to have measurable apparent diameters, the distances of the stars could not explain this weak light. ‘Will my opponent tell me that the stars are very far away from us?’ Kepler wrote (Kepler, Reference Kepler1965: 35), ‘This does not help his cause at all. For the greater their distance, the more does every single one of them outstrip the sun in diameter’. Stars had to be huge, given their measured apparent sizes and their vast distances from Earth as required by the Copernican system (which Kepler strongly supported) absent detectable stellar parallax. In 1604, Kepler had calculated that Sirius surpassed the orbit of Saturn in size. Every single star visible to the eye had to surpass the orbit of Earth (Fig. 1) – and be far dimmer than the sun (Graney, Reference Graney2019; Kepler, Reference Kepler2021).

Figure 1. Diagram of the universe of stars from Johannes Kepler's Epitome of Copernican Astronomy, showing a small sun (the dot at the centre) surrounded by large stars.

The stars simply were not suns (Koyré, Reference Koyré1957: 63–86): ‘Our sun’, Kepler wrote in the Conversation (Kepler, Reference Kepler1965: 43), ‘is more splendid than the fixed stars’. Kepler made it clear that Bruno's ideas had no basis in science. Every astronomer could make basic measurements, do simple math and reproduce Kepler's results to see that Bruno was wrong and there was only one sun (Graney, Reference Graney2019).

A plurality of worlds

The universe we envision today is closer to Bruno's than to Kepler's. We search for intelligent life on other earths orbiting other suns, not on Jupiter. Bernard Le Bovier de Fontenelle promoted the idea of other earths with his 1686 book, Conversations on the Plurality of Worlds. Its frontispiece, by Juan d'Olivar, showed the solar system as but one system among many (Fig. 2). ‘French society was shocked’, says historian Lucía Ayala (Ayala, Reference Ayala2012) and ‘this shock quickly spread throughout Europe’.

Figure 2. Frontispiece to Fontenelle's 1686 Conversations on the Plurality of Worlds.

Plurality discussed how the moon must be inhabited because it is like the Earth, and the planets, too, because they are like the moon. Invoking the theory of René Descartes, Kepler's younger contemporary, in which vortices in a universal fluid drove orbital motion (Charalampous, Reference Charalampous2019), Plurality supposed the stars, ‘luminous bodies in themselves, and so many suns’, to be vortex centres with their planets. These hosted inhabitants who see the universe just as we do (Fontenelle, Reference Fontenelle1715: 134–141). The universe comprised a ‘plurality of worlds’ like ours.

Fontenelle's reasoning regarding stars being ‘so many suns’ was that ‘their light is bright and shining’ – and twinkling, because of interactions between stellar vortices (Fontenelle, Reference Fontenelle1715: 134, 150). He was apparently unaware that astronomers knew that twinkling is an atmospheric phenomenon; Christoph Scheiner and his student Johann Georg Locher had discussed it thoroughly, seven decades earlier (Scheiner and Locher, Reference Scheiner and Locher2017). Plurality's science here was not rigorous.

However, Ayala argues that Plurality's appeal was political, not scientific. King Louis XIV of France had embraced Copernicanism as a metaphor for his rule as ‘The Sun King’. Ayala writes that he ‘undertook many endeavours to convince others of his own conviction: that natural forces legitimized his power, Copernicanism being his major proof’. She references a flattering preface, written to him in an astronomy book: ‘Indeed, SIRE, you are at the center of this kingdom as the sun, according to the hypothesis of Copernicus, is at the center of the universe’, etc. (italics added). This ‘colonization’ of the sun by Louis XIV, Ayala argues, ‘paved the way for the enthusiastic reception of the idea of the plurality of worlds’, dethroning the sun and diminishing the Sun King. D'Olivar's illustration features a face in every one of the innumerable suns (Fig. 3). Our sun is not special; the universe is not structured around a single, brilliant ruler (Ayala, Reference Ayala, Neuber, Zittel and Rahn2015: 207, 209, 216).

Figure 3. Detail from the Fontenelle frontispiece.

Politics aside, by 1686 the scientific case for Kepler's single, brilliant sun happened to be weakening. Telescopes had once seemingly confirmed the single-sun universe that appealed to Louis XIV. In the first half of the 17th century, various astronomers, including Galileo, Scheiner and Locher, Simon Marius and Giovanni Battista Riccioli, observed stars telescopically (with apertures of 1–2 cm, typically), and recorded them as discs of measurable apparent sizes (Fig. 4). Astronomers were again unaware that these discs were optical artefacts, in fact the Airy discs produced by such small apertures owing to the wave nature of light, a phenomenon unknown at that time.

Figure 4. Illustration of a star as seen through a small-aperture telescope, from John Hershel's Treatises on Physical Astronomy, Light and Sound.

The disc sizes, ~10 arc seconds for the more prominent stars, were substantially smaller than pre-telescopic measurements, but still translated into giant stars in a Copernican universe, especially since telescopes increased sensitivity to parallax. Galileo supported Copernicus, of course, but struggled with the giant star question. Scheiner, Marius and Riccioli all argued for Brahe's Earth-centred model of the universe that accommodated new telescopic discoveries while having stars located just beyond, and thus like in size to, Saturn (Graney, Reference Graney2015: 45–86, 129–139; Graney, Reference Graney2021a).

But by the 1660s, Johannes Hevelius and Christiaan Huygens had published observations (of lunar occultations of stars, and of stellar apparent sizes diminishing with filtering) suggesting that even telescopes greatly inflated stellar sizes. In such a case, stars could be suns. These observations did not go unchallenged, however. For example, John Flamsteed, England's first Astronomer Royal, countered that Sirius and Mercury, seen through the same small aperture telescope under the same conditions, had the same apparent diameters (Applebaum, Reference Applebaum2012; Graney, Reference Graney2015: 148–158). Thus when Fontenelle published Plurality, the science concerning stars being suns was in flux.

But in 1716 and 1740, Jacques Cassini of the Paris Observatory published high-quality telescopic (small aperture) measurements of Sirius's apparent diameter: 5՛՛. He showed Sirius to be giant, granted a Copernican universe. As with Kepler, all stars had to be giant – not suns (Graney, Reference Graney2021b).

Fellow astronomers acknowledged Cassini's measurements, but enthusiasm for a plurality of worlds, or ‘Pluralism’, had caught on – they considered stars to be suns anyway. John Hill borrowed heavily from Cassini in his 1754 book Urania, and wrote how –

Note the emphasis on the reproducibility of Cassini's results. Nevertheless, Hill wrote that each star is a sun, with ‘earthy planets rolling round it’ – because, why else would the stars exist, and doesn't such a universe glorify its Creator? Pluralism apparently had religious appeal for Hill (Hill, Reference Hill1754; Graney, Reference Graney2021b). Whether Pluralism's appeal was political or religious, it was such that high-quality, easily-reproducible telescopic data, even from the esteemed Cassini, would not overcome it.

Of course, in time it would become clear that Huygens was right about star sizes, and Cassini, Flamsteed and Kepler were wrong. Full understanding that telescopic stellar discs were optical artefacts, not stellar bodies, had to await the 19th century, the wave theory of light, and George Biddell Airy (Graney and Grayson, Reference Graney and Grayson2011; Graney, Reference Graney2015: 154–157).

By then Pluralism was broadly accepted; astronomers and others in the early 19th century typically considered every planet in orbit around the sun to be inhabited. William Herschel, the first astronomer to discover a new planet, had even proposed that the sun was inhabited, ‘like the rest of the planets’. ‘Astronomical principles’ showed this, he wrote in 1795, and he was sure he could answer every objection made against his proposal. Thomas Paine in his Age of Reason wrote of the inhabitants of ‘each of the worlds of which our [solar] system is composed’ and of those ‘millions of worlds’ around other stars, also. In the 1830s Thomas Dick even estimated the population of the solar system: tens of trillions (not counting solar inhabitants). The population of the universe? Trillions of times larger still (Crowe, Reference Crowe1986; Crowe, Reference Crowe2008: 179–181, 228–229, 269–271).

A diversity of stars

Once the star size problem was resolved, science ceased to directly challenge Pluralism, but science offered nothing to support it, either. Towards the end of the 19th century, Agnes Clerke described the progress of knowledge about stars during that century. At the century's start, little was known; stars were a background against which astronomers measured planetary motions. ‘The sidereal world… was the domain of far-reaching speculations’ that were unencumbered by systematic study. William Herschel, she noted, assumed that ‘the brightness of a star afforded an approximate measure of its distance’ – one star was more or less the same as another (Clerke, Reference Clerke1908: 11, 21). This meshes with stars being (more or less identical) suns. With so little known about the stars, nothing stood against this assumption, but no science supported it, either.

Yet by the century's end, Clerke wrote, the distances to roughly one hundred stars were known through parallax measurements. Moreover (Clerke, Reference Clerke1908: 37):

Many of the brightest stars had been found to be too remote to measure their distances, while many stars that were found to be nearby were quite faint:

We have learned much since Clerke. Still, her observation holds true. There is great diversity in the universe of stars, from those rare stars that rival the sizes Kepler determined, down to the super-abundant red dwarfs.

A diversity of planets

The 19th century revealed a great diversity among planets, too. The historian of science Michael J. Crowe has argued that William Whewell, Master of Trinity College of Cambridge University, first envisioned this diversity. In 1853, Whewell anonymously published Of the Plurality of Worlds: An Essay, attacking scientifically the idea of a universe widely inhabited with intelligent life (Crowe, Reference Crowe2016).

One of Whewell's key arguments was the inverse-square law; the heat and light a planet receives depends strongly on its distance from the sun. Crowe argues that Whewell was among the first to consider the idea of a ‘habitable zone’ around a star (Whewell used the term ‘temperate zone’). This implied that the rest of the region around a star is not habitable, contrary to William Herschel, Thomas Dick, etc.

Whewell, formerly president of England's Geological Society, also used geology to argue against widespread extraterrestrial intelligence. Crowe writes (Crowe, Reference Crowe2016: 441):

Whewell speculated nevertheless about lower life within the solar system – such as, on Jupiter, ‘aqueous, gelatinous creatures; too sluggish, almost, to be deemed alive, floating on their ice-cold water, shrouded forever by their humid skies (Whewell, Reference Whewell1853: 185–186)’.

Scientific evidence for diverse planets, and not merely other earths, had long been available. The great diversity in planetary sizes had been known for more than two centuries (Fig. 5). Isaac Newton, whose physics supplanted Descartes's vortices, had included in the third edition of his Principia (1726) calculations showing substantial differences among solar system bodies in mass, density and surface gravity (Fig. 6); differences from Earth might have provided reason to suppose that the planets would lack intelligent life (Crowe, Reference Crowe2016).

Figure 5. Sizes of planets and sun, from the 1698 Cosmotheoros of Christiaan Huygens.

Figure 6. Strength of gravity on different bodies, from the 1729 edition of Newton's Mathematical Principles of Natural Philosophy, Volume 2 (p. 227).

Astronomers before Whewell had recognized planetary diversity, but in ways inclined towards Pluralism. Consider the prominent astronomer John Herschel, Whewell's friend and William's son. Prior to Whewell's 1853 Essay, Herschel had discussed Mercury receiving more solar heat than Uranus, Jupiter having stronger gravity than Earth and the density of Saturn being so low that it ‘must consist of materials not much heavier than cork’. Yet he presumed that the planets would be inhabited, much as his father presumed the sun would be inhabited; he marvelled at the ‘Benevolence and Wisdom which presides over all’ the habitable universe, much like Hill (Crowe, Reference Crowe2016: 440). Writing to Whewell in response to the Essay, John Herschel stated that though he had compared Saturn to cork, ‘it never did occur to me to draw the conclusion that ergo the surface of Saturn must be of extreme tenuity’. He then insisted that, even were Jupiter an ice-cold sea, it might be populated by something more than Whewell's gelatinous creatures; intelligent fish might construct ‘crystal palaces’ (referencing the Crystal Palace of the London Great Exhibition of 1851) in the warmer depths of the Jovian seas (Crowe, Reference Crowe2008: 358–359).

But this inclination towards Pluralism was running into more scientific difficulties in the 19th century than just the inverse-square law and geological timescales. The idea that life spontaneously generated from matter, which would make Jovian fish or even life on the sun reasonable, was being overthrown.

This idea dated back to at least Aristotle. Frogs were thought to be generated right out of the mud (Deichmann, Reference Deichmann2012); an ancient poet wrote of how ‘feetlesse and without legs on earth they lie (Topsell, Reference Topsell1658: 719–720)’. Ancient Jewish Rabbis discussed whether the earth from which a mouse might be spontaneously forming would be unclean, since Leviticus 11:29 lists mice as being among the various ‘creeping things’ that are unclean (van der Horst, Reference van der Horst1993/94). Kepler remarked on how the Earth ‘kindles daily so many little living things from herself – plants, fishes, insects (Kepler, Reference Kepler2021: 58)’ – and he apparently supposed that Jupiter kindled them, too. As late as the 1880s, the botanist Carl Nägeli argued for the spontaneous generation of the simplest living organisms, with higher life forms evolving from those (Mason, Reference Mason1962: 428–31; Farley, Reference Farley1972). But by the end of the 19th century science had rejected spontaneous generation entirely (Deichmann, Reference Deichmann2012). Indeed, science today is very far from spontaneous generation, theorizing that life on Earth originated long ago, through a process neither reproducible in a lab nor found re-occurring in nature, and that more complex life originated in a merger of two primitive, single-celled organisms – a merger that occurred once in Earth's history, and only after primitive life had existed for many hundreds of millions of years (Lane, Reference Lane2015).

So we do not expect to find life on the sun or Jupiter. Even one small colony of microscopic gelatinous creatures in the dark, ice-cold waters of Enceladus would be a monumental find. Solar system bodies differ from Earth. Exoplanets show us further diversity, with planets larger than Jupiter in orbits smaller than Mercury's, and with planets of sizes unlike any found in our system. Whewell was right about planetary diversity, beyond his own expectations.