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Webb narrows atmospheric possibilities for Earth-sized exoplanet TRAPPIST-1 d

The exoplanet TRAPPIST-1 d intrigues astronomers looking for possibly habitable worlds beyond our solar system because it is similar in size to Earth, rocky, and resides in an area around its star where liquid water on its surface is theoretically possible. But according to a new study using data from the NASA/ESA/CSA James Webb Space Telescope, it does not have an Earth-like atmosphere.

A protective atmosphere, a friendly Sun, and lots of liquid water — Earth is a special place. Using the unprecedented capabilities of the Webb, astronomers are on a mission to determine just how special, and rare, our home planet is. Can this temperate environment exist elsewhere, even around a different type of star? The TRAPPIST-1 system provides a tantalizing opportunity to explore this question, as it contains seven Earth-sized worlds orbiting the most common type of star in the galaxy: a red dwarf.

“Ultimately, we want to know if something like the environment we enjoy on Earth can exist elsewhere, and under what conditions. While the James Webb Space Telescope is giving us the ability to explore this question in Earth-sized planets for the first time, at this point we can rule out TRAPPIST-1 d from a list of potential Earth twins or cousins,”

said Caroline Piaulet-Ghorayeb of the University of Chicago and Trottier Institute for Research on Exoplanets (IREx) at Université de Montréal, lead author of the study published in The Astrophysical Journal.

Planet TRAPPIST-1 d

The TRAPPIST-1 system is located 40 light-years away and was revealed as the record-holder for most Earth-sized rocky planets around a single star in 2017, thanks to data from NASA’s retired Spitzer Space Telescope and other observatories. Due to that star being a dim, relatively cold red dwarf, the “habitable zone” – where the planet’s temperature may be just right, such that liquid surface water is possible – lies much closer to the star than in our solar system. TRAPPIST-1 d, the third planet from the red dwarf star, lies on the cusp of that temperate zone, yet its distance to its star is only 2 percent of Earth’s distance from the Sun. TRAPPIST-1 d completes an entire orbit around its star, its year, in only four Earth days.

Webb’s NIRSpec (Near-Infrared Spectrograph) instrument did not detect molecules from TRAPPIST-1 d that are common in Earth’s atmosphere, like water, methane, or carbon dioxide. However, Piaulet-Ghorayeb outlined several possibilities for the exoplanet that remain open for follow-up study.

“There are a few potential reasons why we don’t detect an atmosphere around TRAPPIST-1 d. It could have an extremely thin atmosphere that is difficult to detect, somewhat like Mars. Alternatively, it could have very thick, high-altitude clouds that are blocking our detection of specific atmospheric signatures — something more like Venus. Or, it could be a barren rock, with no atmosphere at all,” Piaulet-Ghorayeb said.

The star TRAPPIST-1

No matter what the case may be for TRAPPIST-1 d, it’s tough being a planet in orbit around a red dwarf star. TRAPPIST-1, the host star of the system, is known to be volatile, often releasing flares of high-energy radiation with the potential to strip off the atmospheres of its small planets, especially those orbiting most closely. Nevertheless, scientists are motivated to seek signs of atmospheres on the TRAPPIST-1 planets because red dwarf stars are the most common stars in our galaxy. If planets can hold on to an atmosphere here, under waves of harsh stellar radiation, they could, as the saying goes, make it anywhere.

“Webb’s sensitive infrared instruments are allowing us to delve into the atmospheres of these smaller, colder planets for the first time,” said Björn Benneke of IREx at Université de Montréal, a co-author of the study. “We’re really just getting started using Webb to look for atmospheres on Earth-sized planets, and to define the line between planets that can hold onto an atmosphere, and those that cannot.”

The outer TRAPPIST-1 planets

Webb observations of the outer TRAPPIST-1 planets are ongoing, which hold both potential and peril. On the one hand, Benneke said, planets e, f, g, and h may have better chances of having atmospheres because they are further away from the energetic eruptions of their host star. However, their distance and colder environment will make atmospheric signatures more difficult to detect, even with Webb’s infrared instruments.

“All hope is not lost for atmospheres around the TRAPPIST-1 planets,” Piaulet-Ghorayeb said. “While we didn’t find a big, bold atmospheric signature at planet d, there is still potential for the outer planets to be holding onto a lot of water and other atmospheric components.”

Our detective work is just beginning. While TRAPPIST-1 d may prove a barren rock illuminated by a cruel red star, the outer planets TRAPPIST-1e, f, g, and h, may yet possess thick atmospheres,” added Ryan MacDonald, a co-author of the paper, now at the University of St Andrews in the United Kingdom, and previously at the University of Michigan. “Thanks to Webb we now know that TRAPPIST-1 d is a far cry from a hospitable world. We’re learning that the Earth is even more special in the cosmos.”

Illustration of a planet silhouetted in front of a star. The star shows a large eruption on one side and more wisps of red coming from its southern hemisphere. Two more planets appear in the background.
The James Webb Space Telescope narrows atmospheric possibilities for Earth-sized rocky exoplanet TRAPPIST-1 d. This artist’s concept depicts planet TRAPPIST-1 d passing in front of its turbulent star, with other members of the closely packed system shown in the background.
The TRAPPIST-1 system is intriguing to scientists for a few reasons. Not only does the system have seven Earth-sized rocky worlds, but its star is a red dwarf, the most common type of star in the Milky Way galaxy. If an Earth-sized world can maintain an atmosphere here, and thus have the potential for liquid surface water, the chance of finding similar worlds throughout the galaxy is much higher. In studying the TRAPPIST-1 planets, scientists are determining the best methods for separating starlight from potential atmospheric signatures in data from the NASA/ESA/CSA James Webb Space Telescope. The star TRAPPIST-1’s variability, with frequent flares, provides a challenging testing ground for these methods.
Credit: NASA, ESA, CSA, J. Olmsted (STScI)

Bibliographic information:

Caroline Piaulet-Ghorayeb et al.,  ApJ 989 181 2025, DOI: 10.3847/1538-4357/adf207

 

Press release from ESA Webb.

Researcher retrieved archival information that attributes a pseudonymous astronomical treatise to Galileo Galilei

A researcher at the Department of Philosophy and Cultural Heritage of Ca’ Foscari University of Venice, Dr Matteo Cosci, has retrieved archival information which confirms that the treatise Considerazioni Astronomiche di Alimberto Mauri (1606) was in fact written by Galileo Galilei, the illustrious mathematician from Pisa. Galileo used a pseudonym and the author’s uncertain identity had not been confirmed until now. Dr Cosci closely examined original documents preserved at the National Central Library of Florence for the purpose.

Frontespizio delle Considerazioni Astronomiche di Alimberto Mauri (1606), attribuite a Galileo Galilei
Book front page

Not only forged documents

Before this discovery was made, the New York Times had revealed that some of Galileo’s documents held at the University of Michigan and at Morgan Library in New York City were in fact counterfeits made by the infamous forger Tobia Nicotra in the early 20th century. Professor Nick Wilding of Georgia State University, who discovered the counterfeit, demonstrated that the filigree of the paper that the texts were written on cannot predate the 18th century.

When these documents were authenticated at the start of the 20th century, the authentication process was based on other documents attributed to Galileo, which were subsequently revealed to also be forgeries. One of such documents was a counterfeit letter signed by Galileo that was thought to accompany a book entitled “Libro della Considerazione Astronomica”. Starting in the late 1970s, in order to explain the reasons behind this letter, scholars hypothesised that the accompanying letter was proof that Galileo had actually written a controversial treatise, Considerazioni Astronomiche di Alimberto Mauri. This treatise was known to have been written under pseudonym, and since its publication in 1606 it had been attributed by some to Galileo himself. For one, Fortunio Liceti — Galileo’s colleague at the University of Padua — referred to Aliberto Mauri as someone who “pretended” to be an astronomer though he might rather have been an expert mathematician.
However, the true identity of the author was never established with certainty. In the view of some scholars, the accompanying letter — which is currently hosted in the Fondo “Cardinale Pietro Maffi” in Pisa — seemed to confirm that Galileo was indeed the author of the Considerazioni Astronomiche. Despite the fact that now the only document which seemed to support the ascription of authorship to Galileo has been declared falsethe emergence of different original documents makes this identification certain.

The retrieval

Matteo Cosci found important information among the papers in the collection “Gal. 42” at Biblioteca Nazionale Centrale di Firenze, which contains Galileo’s Frammenti e primi abbozzi relativi al trattato galileiano “Delle cose che stanno su l’acqua”. On the whole, these handwritten papers are a collection of notes taken in different periods of time and on different topics, including some references to the “stella nova” (new star) of 1604 that diverge from the interpretation that at the time was being given by the Florentine philosopher Lodovico Delle Colombe.

Matteo Cosci

Even though they were not about the same topic, Galileo’s brief notes on the “new star” were evidently collected together with his others about the floating bodies because they were addressed against the same opponent. Dr Cosci noticed both their apparent misplacement and their peculiarity while he was systematically examining all the handwritten drafts of Galileo on the “new star” dispute. Previous cataloguing of this material had already confirmed that it was written by Galileo in opposition to Lodovico Delle Colombe’s writings. However, these notes had never been considered relevant enough to be included in the national edition of Galileo’s work — in fact, they remain unpublished.

Among these papers by Galileo, on page 31 recto, there is a list of “places where [Lodovico Delle Colombe] speaks of me with contempt.” Dr Cosci noticed that those “places” are precise references to some selected textual passages in Lodovico Delle Colombe’s Risposte (i.e. Answers). Then he realised that those passages do not openly attack Galileo (who is never even mentioned), but do attack Alimberto Mauri. The fact that Galileo felt personally “attacked” whenever Alimberto Mauri was attacked in print confirms that Alimberto Mauri was his alter ego. Simply put, in these private notes, Galilei himself reveals his identity as the one hiding behind a pseudonym.

Overall, the autographic documents examined by Matteo Cosci are currently the only authentic piece of documentary evidence that enables the attribution of Considerazioni Astronomiche to Galileo.

Why did Galileo use a pseudonym?

Galileo was successfully working in Padua, but his salary no longer suited his own needs and his family requirements. As Stillman Drake previously hypothesised, Galileo published this treatise in an attempt to find patronage beyond the borders of the Venetian Republic, and more specifically in Rome — in fact, the treatise was dedicated to none other than the Pope’s Treasurer. However, those were the years of the Venetian Interdict (a diplomatic quarrel between the Papal Curia and the Republic of Venice), so it would have been unwise of Galileo to place his name on a treatise that was dedicated to the public enemy.

Galilei had used pseudonyms before. He had participated with the assistance of one of his students in a debate on the same star using the pseudonym “Cecco da Ronchitti”. In fact, Lodovico Delle Colombe indirectly addressed Galileo as “la Signora maschera” (i.e. Mr. Mask), “Mauri”, “Cecco”, and “quel dottor che leggeva in Padova” (i.e. “that professor that was a lecturer in Padua”). Delle Colombe subsequently wrote his Risposte keeping Galileo in mind, but hesitating to openly identify his adversary. This, too, contributed to the general sense of uncertainty over authorship. Another note discovered by Dr Cosci shows that that Galileo initially wanted to reply further to Lodovico Delle Colombe, but he concluded that in the end the opponent did not even deserve his time. Nevertheless, the dispute between Galileo and Lodovico Delle Colombe continued and escalated during the first years of Galilei’s stay in Florence, when the use of a pseudonym was no longer necessary for the by then famous author of the Sidereus Nuncius.

Conclusions

The radical re-examination of these unpublished documents has confirmed the attribution of Considerazioni astronomiche to Galileo Galilei. The treatise — a new edition of which is being prepared by Dr Cosci — shows textual similarities with other writings of Galileo on different topics and from different periods of time, such as De MotuConsiderazioni circa l’opinione copernicana, and Dialogo di Cecco da Ronchitti, as well as with a postilla on his copy of Delle Colombe’s text on the new star. Moreover, at the time of the debate, the student Willem van Thienen had added in plain the name “Galileo Galilei” on his copy of Risposte, just below the title “certa maschera saccente nominata Alimberto Mauri” (“a knowing mask named Alimberto Mauri”).

Professor Nick Wilding has commented:

‘This is an excellent example of how patient and intelligent archival research can restore some of the damage inflicted by forgers. Dr Cosci has shown us that a combination of scepticism and skill will lead us to historical truth.’

In addition, Prof. Peter Barker (University Of Oklahoma),who has been aware of Cosci’s research, claimed:

Sidereus Nuncius tells us when, how and what Galileo made telescopic observations about. But the perspective of Considerazioni Astronomiche shows uswhyhe made those observations three years later.’

In sum, a new chapter can be added to the monumental collection of writings by the person who revolutionised Western science. Among the most interesting arguments in this work can be listed, for instance, the hypothesis of existence of mountains on the surface of the moon from a purely perspectivist point of view, the idea that physical causes are the actual reasons for explaining the regularity of celestial motions that apparently follow nonuniform paths, and the criticism of those who reject astrology without having the necessary astronomical knowledge to properly do so.

Therefore, Considerazioni Astronomiche di Alimberto Mauri is written by an unusual, yet recognisable Galileo, during a transition phase in which he was at once looking for new patronage and trying to confute the most retrograde Aristotelian tenets, just a few years before his discoveries with the telescope would lead him to move to Florence and then make him famous all over the world. For that matter, the printing privilege informs us that the treatise was published in Florence with the assent of Paolo Vinta, prime secretary of the Grand Duchy and brother of Belisario, who was in turn Galileo’s friend, correspondent and shortly afterwards mediator for his desired rerturn in Tuscany.

The study leading to this result was originated within the ERC research project “Aristotle in the Italian Vernacular: Rethinking Renaissance and Early-Modern Intellectual History (c. 1400–c. 1650)” , and that is currently being pursued at Ca’ Foscari in partnership with the Department of History of Science, Technology, and Medicine of the Università of Oklahoma within the Marie Skłodowska-Curie project “The Ophiucus Supernova: Post-Aristotelian stargazing in the European context (1604-1654)”, which Dr Cosci is responsible for.

Bibliographic information:

– 15/07/2022: Matteo Cosci, “Galileo’s pseudonymous project for his treatise on the ‘Stella Nova’ of 1604”, Department of History of Science, Technology, and Medicine, University of Oklahoma; Norman, Oklahoma.
– 24/03/2022: Matteo Cosci, “Galileo alias Alimberto Mauri: nuove evidenze documentarie per una nuova edizione delle Considerazioni”, Project Workshop, “Teorie e pratiche astrologiche al tempo di Galileo Galilei”, with Elide Casali and Monica Azzolini (Discussant: H. Darell Rutkin), Aula Morelli/Biral, Malcanton Marcorà, Dipartimento di Filosofia e Beni Culturali, Venice Ca’ Foscari University. https://www.unive.it/data/33113/1/59122

 

Press release from Ca’ Foscari University of Venice