AstroKobi
Space · Astronomy · Wonder
astronomyFriday, July 17, 2026·3 min read

The Roman Space Telescope Will Find Ancient Black Holes By Watching How They Eat Stars

The Roman Space Telescope will detect ancient black holes by observing tidal disruption events, helping scientists understand how supermassive black holes grow.

Dramatic CGI rendering of a black hole with swirling accretion disk.
Photo: Adis Resic

The Roman Space Telescope is set to revolutionize our understanding of ancient black holes by observing how they consume stars. When a star gets too close to a supermassive black hole (SMBH), the black hole's tidal force tears the star apart, creating a tidal disruption event (TDE). This event makes the SMBH detectable, as the stellar material heats up and becomes extremely luminous.

What happened

Researchers have predicted how many TDEs the Roman Space Telescope and other powerful telescopes will detect. The study, titled "Tidal Disruption Event Rates across Cosmic Time: Forecasts for LSST, Roman, and JWST and Their Constraints on the Supermassive Black Hole Mass Function," focuses on detecting lower-mass SMBHs, which are difficult to observe. TDEs are one of the few ways to detect these lower-mass SMBHs, which have masses between 100 thousand and 100 million solar masses.

The Roman Space Telescope's High-Latitude Time Domain Survey (HLTDS) will regularly observe the same region of the sky, allowing it to detect TDEs and study the population of lower-mass SMBHs across cosmic time. This will help scientists understand how SMBHs grow and evolve over billions of years.

Why it matters

Understanding the growth of supermassive black holes is crucial, as they play a significant role in the evolution of galaxies. By detecting TDEs, scientists can gain insights into the mass distribution of SMBHs over cosmic time, particularly for the low-mass population at high redshifts.

+ Pros
  • The Roman Space Telescope will detect TDEs, allowing scientists to study the population of lower-mass SMBHs.
  • Understanding the growth of SMBHs will shed light on the evolution of galaxies.
  • TDEs provide a unique way to detect lower-mass SMBHs.
Cons
  • Detecting TDEs is challenging, requiring powerful telescopes like the Roman Space Telescope.
  • The study of SMBHs is complex, requiring the analysis of large amounts of data.
  • The low-mass population of SMBHs is difficult to observe.

How to think about it

To understand the significance of the Roman Space Telescope's mission, consider the role of supermassive black holes in galaxy evolution. By studying TDEs, scientists can gain insights into the growth and evolution of SMBHs over billions of years.

FAQ

What is a tidal disruption event?+
A tidal disruption event (TDE) occurs when a star gets too close to a supermassive black hole, causing the black hole's tidal force to tear the star apart.
Why is it difficult to detect lower-mass SMBHs?+
Lower-mass SMBHs are difficult to detect because they do not emit significant amounts of radiation, making them invisible to most telescopes.
How will the Roman Space Telescope detect TDEs?+
The Roman Space Telescope's High-Latitude Time Domain Survey (HLTDS) will regularly observe the same region of the sky, allowing it to detect TDEs and study the population of lower-mass SMBHs.
Sources
  1. 01The Roman Space Telescope Will Find Ancient Black Holes By Watching How They Eat Stars
  2. 02The Roman Space Telescope Will Find Ancient Black Holes By Watching How They Eat Stars
Keep reading