Fishing with LSST in the Ocean of Interstellar Space

Avi Loeb
6 min readAug 14, 2024

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A drone view of the Rubin Observatory at sunset in May 2024 on Cerro Pachón in Chile. (Image credit: NOIRLab)

Genuine scientists, who are curious and wish to learn something new about the physical reality, are eager to study as much data as possible. Fake scientists do not want their past beliefs to be disproven by new facts, and so they sweep anomalous data under the carpet of past knowledge and resist more data. Less data helps their state of mind, since new anomalies trigger a cognitive dissonance in which they are forced to consider simultaneously two contradictory notions. This is what I thought after hearing a leading astronomer who specializes in the solar system, say: “`Oumuamua is so weird. I wish it never existed.”

How can we get more data on `Oumuamua-like objects? By constructing a new discovery machine at a cost of 1.9 billion dollars. This unprecedented observatory is becoming a reality thanks to funding from the National Science Foundation and the U.S. Department of Energy.

On July 24, 2024, the Rubin Observatory’s 3.5-meter secondary mirror was installed as the first piece of glass placed at its final position on the telescope. The observatory is planned to see first light in 2025, when it will begin the Legacy Survey of Space and Time (LSST). The telescope will image the entire southern sky every 4 days using a camera with 3.2 billion pixels, a thousandfold increase relative to cell phone cameras. It will capture the highest-resolution video of the entire sky, producing the longest silent movie ever created of the Universe for ten years.

The Rubin Observatory site enjoys an average of 256 clear nights a year. Upon arrival to Chile, the secondary mirror was coated in 2019 by silver for its superior reflectivity. The secondary mirror assembly was placed into position on the telescope structure. Once it was securely attached, the electronics were connected and the software control system was activated. Next on the installation schedule, a temporary Commissioning Camera will test the system. Subsequently, the 8.4-meter primary/tertiary mirror assembly will be integrated. This will be followed by the final installation of the LSST camera — the largest digital camera in the world, which is about the size of a compact car and weighs about 3 tons. The LSST camera will have a field of view of 9.6 square degrees. Each image will contain two 15 second exposures. Over 10 years LSST will generate a staggering 60 petabytes of data, 6 million gigabytes per year.

It is estimated that LSST will monitor 20 billion galaxies, 17 billion individually resolved stars, and the orbits of more than 5 million objects within our Solar System.

On July 24, 2024, Rubin Observatory’s 3.5-meter secondary mirror was installed. (Image credit: NOIRLab)

Among the 5 million objects in the Solar System, astronomers expect at least several tens of interstellar objects like `Oumuamua and interstellar comets like Borisov. LSST could also reveal a few interstellar meteors like IM1, as well as Unidentified Anomalous Phenomena (UAP) which may appear different than the known populations of human-made satellites or space trash by the way they maneuver.

Beyond discovering new objects, the Rubin Observatory will also usher in a revolution in time-domain data. LSST will monitor most Solar System objects over a ten-year period, with likely hundreds of observations per object split across 6 broad-band (u,g,r,I,z,y) filters. The large number of observations per object will allow study of rotational light curves and colors which probe the shape, size, rotation rate, and surface composition of the objects. Follow-up observations by the Webb telescope will provide additional information on the objects’ surface temperature, size, albedo of sunlight, cometary tail, 3D location versus time, and non-gravitational acceleration — based on the parallax relative to telescopes on Earth.

LSST could also track the population of killer asteroids or comets that could endanger our civilization. As of now, we are only aware of about 40% of near-Earth objects larger than 100 meters, roughly the size of `Oumuamua, that can cause continent-wide destruction by impacting Earth. The Rubin Observatory could increase the known fraction to 80% and improve the prospects for planetary defense by developing plans to slightly deflect dangerous objects, decades in advance. One approach for defense is to send spacecraft that will collide with a hazardous object, as demonstrated by NASA’s DART spacecraft which collided with the asteroid moonlet Dimorphos on September 26, 2022. Another approach is to shine a laser beam and ablate one side of the object, so as to propel it away from Earth by the rocket effect of the evaporated gas. Finally, there is a possibility of painting one side so that the reflection of sunlight would push the object away from Earth. The farther is the object from Earth, the smaller is the required deflection.

Together with my Laukien-Oumuamua postdoc in the Galileo Project, Richard Cloete, and astronomer Peter Vereš, we are currently developing the software needed to identify potential interstellar objects in the LSST data pipeline. Here’s hoping that future LSST data will flag extraterrestrial technological debris as anomalous among the expected population of interstellar asteroids or comets produced by nature. Such a finding will establish a new frontier of astro-archaeology, allowing humans to study the history of Milky-Way civilizations that may have existed billions of years ago.

The tombstones in the graveyard of the Milky-Way inform us about its past. From the age distribution of white dwarfs, the remnants of sun-like stars, it is possible to infer the stellar birth rate in the past. The inferred history of the Milky-Way disk includes a peak of star formation ten billion years ago, followed by a constant star formation rate of a few sun-like stars every year. The Sun formed 4.6 billion years ago, half way in lookback time to the peak in the star formation rate. The peak reached a level that was 3 times higher than the subsequent plateau, suggesting that most stars formed several billion years before the Sun. With cosmic modesty as our guiding principle after the Copernican revolution, this suggests that technological objects similar to our own interstellar probes could have reached us from the other side of the Milky-Way disk by now. This realization was demonstrated by detailed calculations in a new paper that I wrote with my undergraduate student, Shokhruz Kakharov.

A large enough statistical sample of the arrival directions and velocities of interstellar objects would allow us to infer the possible origin and age of these objects in the Milky-Way galaxy.

The forthcoming decade of discovery enabled by the Rubin Observatory could inform us that we are not alone. I am often asked what would constitute clear evidence beyond a reasonable doubt for an extraterrestrial technological object, to which I reply: “high-quality data on an object with a shape, composition and dynamics that do not resemble familiar rocks and human-made gadgets.”

Discovering conclusive evidence for interstellar technological debris with LSST would remind us that we are not alone. As earthlings, we all share the same boat as we travel through the ocean of interstellar space. We better cooperate as “team Earth” when we discover trash from other boats that travelled before us in this ocean.

Scientific discovery can be exciting if we explore what lies beyond the horizon without insisting that we know the answer in advance. The sky’s the limit for our imagination. This is the motivation for the Galileo Project expedition to the Pacific Ocean within the coming year, to retrieve large pieces of the interstellar meteor, IM1. In combination with the inauguration of LSST, the year 2025 is going to be a good vintage year for interstellar discoveries.

View of Rubin Observatory at sunset in May 2024. (Image credit: NOIRLab)

ABOUT THE AUTHOR

(Image credit: Chris Michel, 2023)

Avi Loeb is the head of the Galileo Project, founding director of Harvard University’s — Black Hole Initiative, director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, and the former chair of the astronomy department at Harvard University (2011–2020). He is a former member of the President’s Council of Advisors on Science and Technology and a former chair of the Board on Physics and Astronomy of the National Academies. He is the bestselling author of “Extraterrestrial: The First Sign of Intelligent Life Beyond Earth” and a co-author of the textbook “Life in the Cosmos”, both published in 2021. His new book, titled “Interstellar”, was published in August 2023.

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Avi Loeb
Avi Loeb

Written by Avi Loeb

Avi Loeb is the Baird Professor of Science and Institute director at Harvard University and the bestselling author of “Extraterrestrial” and "Interstellar".