Cosmic Giants: The Role of Supermassive Black Holes in Galaxy Evolution | Cosmos in a Pod S1E37 episode artwork

EPISODE · Dec 19, 2024 · 21 MIN

Cosmic Giants: The Role of Supermassive Black Holes in Galaxy Evolution | Cosmos in a Pod S1E37

from Cosmos in a Pod

Welcome to Cosmos in a Pod! I’m your host, Amitesh, and today we’re diving into the heart of galaxies—literally. Supermassive black holes, the colossal gravitational engines at the centres of most large galaxies, are more than just cosmic devourers. These mysterious giants shape their galaxies, regulate star formation, and power some of the brightest phenomena in the universe.Episode HighlightsWhat Are Supermassive Black Holes?Definition: Black holes millions to billions of times the mass of the Sun.Key Features: Event horizon, accretion disk, and relativistic jets.Notable Examples:Sagittarius A*: The Milky Way’s relatively quiet SMBH (~4 million solar masses).M87’s Black Hole: The first-ever imaged black hole, with a mass of ~6.5 billion Suns.TON 618: Among the most massive black holes, with over 66 billion solar masses.How Do SMBHs Form?Direct Collapse: Massive gas clouds collapse directly into black holes.Growth via Accretion: Smaller black holes accumulate matter over billions of years.Mergers: Black holes grow through galaxy mergers and coalescing with other black holes.Primordial Black Holes: Black holes formed shortly after the Big Bang may have seeded SMBHs.The Role of SMBHs in Galaxy EvolutionRegulating Star Formation:Quasar Mode Feedback: Intense energy output prevents gas from forming stars.Radio Mode Feedback: Steady jets heat surrounding gas, suppressing star formation.Fueling Quasars and Active Galactic Nuclei (AGN):Accretion disks emit vast amounts of radiation, powering quasars visible across billions of light-years.Shaping Galactic Structures:Influence the formation of central bulges and galaxy morphology, especially during mergers.How Do We Observe Supermassive Black Holes?Motion of Stars and Gas: Detecting the Gravitational Effects on Nearby Objects.Accretion Disk Radiation: Emissions in X-rays, UV, and visible light.Gravitational Waves: Ripples in spacetime from merging SMBHs, observed by LIGO and VIRGO.Imaging: The Event Horizon Telescope provided the first image of a black hole’s shadow in 2019.Unanswered Questions About SMBHsHow do SMBHs grow so quickly, especially in the early universe?What role does dark matter play in their formation and growth?Are intermediate-mass black holes the missing link between stellar-mass black holes and SMBHs?The Cosmic PerspectiveSupermassive black holes are not just destructive entities; they are architects of the universe. By regulating star formation, shaping galaxy structures, and powering luminous quasars, SMBHs play a central role in the life cycle of galaxies. They remind us that even in their immense gravity, these cosmic giants are engines of creation and evolution.

Episode metadata supplied by the publisher feed · Published Dec 19, 2024

Embed this episode

NOW PLAYING

Cosmic Giants: The Role of Supermassive Black Holes in Galaxy Evolution | Cosmos in a Pod S1E37

0:00 21:33

No transcript for this episode yet

We transcribe on demand. Request one and we'll notify you when it's ready — usually under 10 minutes.

No similar episodes found.

No similar podcasts found.

Frequently Asked Questions

How long is this episode of Cosmos in a Pod?

This episode is 21 minutes long.

When was this Cosmos in a Pod episode published?

This episode was published on December 19, 2024.

Is there a transcript available for this episode?

Yes, a full transcript is available for this episode. You can read the complete transcript on the episode page.

Can I download this Cosmos in a Pod episode?

Yes. Use the download control on the episode player to save the publisher-provided media file.
URL copied to clipboard!