Richard D’Souza

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This is a collection of articles archived for the excellence of their content.

The man

Nigel Britto, July 29, 2018: The Times of India

Science and faith are two very fundamental ways of knowing the same reality, says Richard D’Souza
From: Nigel Britto, July 29, 2018: The Times of India

Around two billion years ago, Andromeda, the largest galaxy in our celestial neighbourhood, embarked on an ambitious merger and acquisition project, walloping M32p, a long-lost sibling of our own galaxy, the Milky Way, in an act of celestial cannibalism that left behind a rich trail of evidence — a halo of stars larger than the unimaginably large Andromeda itself, and a mysterious satellite galaxy.

This was recently discovered by a team of University of Michigan researchers led by Richard D’Souza from Pilerne, a small village 8km from Panaji. Growing up in Goa in the 90s, D’Souza couldn’t have imagined that he would soon be solving celestial crimes involving astronomical distances that would make headlines around the world — and all this, as a Jesuit priest.

D’Souza in footsteps of Jesuit scientists

So, when not celebrating mass or ministering to the faithful, Fr D’Souza studies how galaxies grow through mergers. “Over the course of its lifetime, Andromeda is thought to have merged with hundreds of smaller galaxies,” he told STOI from Michigan. “These smaller galaxies are destroyed in the process, leaving behind a trail of stellar debris around the main galaxy, called its stellar halo.”

It has long been known that stellar halos comprise the remnants of small galaxies cannibalised by larger ones. But it has also long been thought it would be difficult to learn about any single one — that is, until D’Souza and his colleague Eric Bell, of the university’s department of astronomy, used computer simulations to deduce most of the stars came from the shredding of one galaxy.

“It’s similar to guessing what a small child has eaten after looking at the crumbs and mess scattered on the floor,” D’Souza said. D’Souza and Bell published their findings in the peer-reviewed journal Nature Astronomy.

Pune-born D’Souza, 40, spent his initial years in Kuwait before studying at St Britto’s High School and St Xavier’s College in Mapusa. Later, amid the intellectual rigour of Jesuit training, which included degrees in philosophy and theology, he got a bachelor’s degree in physics from St. Xavier’s, Mumbai, a master’s in physics from the University of Heidelberg, Germany, and a PhD in astronomy from Ludwig Maximilian University, Munich, before joining the Vatican Observatory and then the University of Michigan for post-doc research.

While many would wonder at the seeming dichotomy of a Catholic priest at the pinnacle of science, D’Souza sees no contradiction. In this, he follows in the footsteps of Jesuit scientists like Fr George Lemaitre, who proposed what came to be known as the Big Bang Theory.

“For me, science and faith are two very fundamental ways of knowing the same reality,” D’Souza said. “It is important to realise science is based on assumptions and faith. Especially in astronomy, where it is very difficult to prove something precisely, it always surprises me how much really depends on assumptions and beliefs.”

Not surprisingly for a Catholic priest, D’Souza, and his science, are fuelled by faith. “Science cannot offer us meaning in life,” he said. “Only something that is totally transcendental can do that, like the divine.”

“Science cannot provide us meaning. Religion and faith do, and it often gives us a pretty good reason to do good science, because it becomes an expression of reaching out to this transcendent, that is, God.”

For me, science and faith are two very fundamental ways of knowing the same reality

His discovery

Morgan Sherburne, The Milky Way’s long-lost sibling finally found, July 23, 2018: University of Michigan

In this image, the Andromeda galaxy shreds the large galaxy M32p, which eventually resulted in M32 and a giant halo of stars. Credit: Richard D’Souza. Image of M31 courtesy of Wei-Hao Wang. Image of stellar halo of M31 courtesy of AAS/IOP.
From: Morgan Sherburne, The Milky Way’s long-lost sibling finally found, July 23, 2018: University of Michigan

ANN ARBOR—Scientists at the University of Michigan have deduced that the Andromeda galaxy, our closest large galactic neighbor, shredded and cannibalized a massive galaxy two billion years ago.

Even though it was mostly shredded, this massive galaxy left behind a rich trail of evidence: an almost invisible halo of stars larger than the Andromeda galaxy itself, an elusive stream of stars and a separate enigmatic compact galaxy, M32. Discovering and studying this decimated galaxy will help astronomers understand how disk galaxies like the Milky Way evolve and survive large mergers.

This disrupted galaxy, named M32p, was the third-largest member of the Local Group of galaxies, after the Milky Way and Andromeda galaxies. Using computer models, Richard D’Souza and Eric Bell of the University of Michigan’s Department of Astronomy were able to piece together this evidence, revealing this long-lost sibling of the Milky Way. Their findings were published in Nature Astronomy.

Scientists have long known that this nearly invisible large halo of stars surrounding galaxies contains the remnants of smaller cannibalized galaxies. A galaxy like Andromeda was expected to have consumed hundreds of its smaller companions. Researchers thought this would make it difficult to learn about any single one of them.

Using new computer simulations, the scientists were able to understand that even though many companion galaxies were consumed by Andromeda, most of the stars in the Andromeda’s outer faint halo were mostly contributed by shredding a single large galaxy.

“It was a ‘eureka’ moment. We realized we could use this information of Andromeda’s outer stellar halo to infer the properties of the largest of these shredded galaxies,” said lead author D’Souza, a postdoctoral researcher at U-M.

This is a family portrait of our local neighborhood of galaxies, called the Local Group as it would have looked more than 2 billion years ago. The missing galaxy, M32p would have been the third largest galaxy in the Local Group after the Andromeda and Milky Way galaxies. Credit: Richard D’Souza; LMC, M33 and M31, courtesy of Wei-Hao Wang; Milky Way, NASA/JPL; M64, NOAO/AURA/NSF.
From: Morgan Sherburne, The Milky Way’s long-lost sibling finally found, July 23, 2018: University of Michigan

“Astronomers have been studying the Local Group—the Milky Way, Andromeda and their companions—for so long. It was shocking to realize that the Milky Way had a large sibling, and we never knew about it,” said co-author Bell, U-M professor of astronomy.

This galaxy, called M32p, which was shredded by the Andromeda galaxy, was at least 20 times larger than any galaxy which merged with the Milky Way over the course of its lifetime. M32p would have been massive, making it the third largest galaxy in the Local Group after the Andromeda and the Milky Way galaxies.

This work might also solve a long-standing mystery: the formation of Andromeda’s enigmatic M32 satellite galaxy, the scientists say. They suggest that the compact and dense M32 is the surviving center of the Milky Way’s long-lost sibling, like the indestructible pit of a plum. “M32 is a weirdo,” Bell said. “While it looks like a compact example of an old, elliptical galaxy, it actually has lots of young stars. It’s one of the most compact galaxies in the universe. There isn’t another galaxy like it.”

The larger disc in this image, galaxy M64, represents what astronomers suspect the M32p galaxy looked like before the Andromeda galaxy cannibalized it nearly 2 billion years ago. The smaller image at the top shows is the M32p’s present-day remnant, the compact elliptical galaxy, M32.
From: Morgan Sherburne, The Milky Way’s long-lost sibling finally found, July 23, 2018: University of Michigan

Their study may alter the traditional understanding of how galaxies evolve, the researchers say. They realized that the Andromeda’s disk survived an impact with a massive galaxy, which would question the common wisdom that such large interactions would destroy disks and form an elliptical galaxy.

The timing of the merger may also explain the thickening of the disk of the Andromeda galaxy as well as a burst of star formation two billion years ago, a finding which was independently reached by French researchers in earlier 2018.

“The Andromeda Galaxy, with a spectacular burst of star formation, would have looked so different 2 billion years ago,” Bell said. “When I was at graduate school, I was told that understanding how the Andromeda Galaxy and its satellite galaxy M32 formed would go a long way towards unraveling the mysteries of galaxy formation.”

The method used in this study can be used for other galaxies, permitting measurement of their most massive galaxy merger, the researchers say. With this knowledge, scientists can better untangle the complicated web of cause and effect that drives galaxy growth and learn about what mergers do to galaxies.

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