Unlocking the Universe: How the Vera C. Rubin Observatory Will Redefine Our Cosmic Perspective

ESA, NASA, K. SHARON/TEL AVIV UNIVERSITY AND E. OFEK/CALTECH

Due to its ability to detect faint objects, Rubin is anticipated to increase the count of known asteroids and comets by a factor of 10 to 100. A significant number of these will be objects exceeding 140 meters in diameter with orbits that pass near Earth’s, indicating potential threats to our planet. Additionally, it will catalog 40,000 newly discovered small icy bodies in the Kuiper Belt, a majorly unexplored zone beyond Neptune where many comets originate, thereby assisting scientists in gaining a better understanding of our solar system’s composition and history.

“We have never had such a vast telescope capturing images so widely and so deeply.”

Anais Möller, astrophysicist, Swinburne University of Technology, Melbourne, Australia

Apart from our solar system, Rubin will observe distinct flickers indicating exoplanets transiting in front of their host stars, leading to brief dimming. It is also expected to discover thousands of new brown dwarfs, faint objects between the size of planets and stars, whose locations in the Milky Way can provide insights into how stellar formation environments influence the characteristics of objects formed therein. It will identify previously unseen dim dwarf galaxies orbiting our own and scrutinize stellar streams, the remnant paths of stars left behind when the Milky Way fragmented similar galaxies.

The facility will also survey far beyond the Milky Way, cataloging approximately 20 billion previously unknown galaxies and mapping their arrangement in sprawling filamentary structures termed the cosmic web. The gravitational influence of dark matter directly impacts the overall shape of this web, and by studying its structure, cosmologists will gather evidence supporting various theories concerning the nature of dark matter. Rubin is expected to witness millions of supernovae and measure their distance from us, serving as a method for gauging the rate of the universe’s expansion. Some researchers propose that dark energy—which is responsible for the accelerated expansion of the cosmos—may have been more intense in the past. Data from more distant, and therefore older, supernovae could assist in affirming or challenging such hypotheses and possibly narrow down the identity of dark energy as well.

SPENCER LOWELL

In virtually every aspect, Rubin will represent a monumental endeavor, highlighting the widespread anticipation among those in the field to witness its operational commencement.

“We have never had such a vast telescope capturing images so widely and so deeply,” Möller states. “That’s an extraordinary opportunity to truly identify phenomena that are changing in the sky and comprehend their underlying physics.”

Adam Mann is a freelance journalist specializing in space and physics, residing in Oakland, California.