Discuss how a supermassive black hole could have formed at the center of our Galaxy.

Short Answer

Expert verified
The supermassive black hole at the center of our galaxy could have formed via direct collapse of gas clouds or through mergers and accretion of smaller black holes or of matter.

Step by step solution

01

Introduction to Black Holes

A black hole is a region in space where the gravitational field is so strong that no matter or radiation can escape from it. The boundary of a black hole is called the event horizon.
02

Understanding Supermassive Black Holes

Supermassive black holes (SMBH) are a type of black hole that are millions to billions of times more massive than our Sun. They are typically found at the centers of galaxies, including our own Milky Way galaxy.
03

Theories of Formation

There are two main theories on the formation of SMBHs. 1. Direct collapse: It's suggested that some SMBHs may have formed from the direct collapse of vast gas clouds. In the early universe, these large gas clouds could have collapsed under their own gravity to form the SMBHs. 2. Mergers and accretion: This theory proposes that SMBHs were formed from smaller black holes that coalesced, or from black holes that gained mass through the accretion of matter.
04

Formation of the Milky Way's SMBH

The specific processes that led to the formation of Sagittarius A*, the SMBH at the center of the Milky Way galaxy, are still not well-defined. However, both theories mentioned before could have contributed to its formation. It could have originated as a smaller black hole that grew by accreting mass from its surroundings, or it could have been the result of early stellar collisions that created a larger, primordial black hole. It's also possible that a combination of these processes happened.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Use the Starry Night Enthusiast \(\mathrm{TM}^{\mathrm{M}}\) program to observe the Milky Way. (a) Display the entire celestial sphere by selecting Favourites \(>\) Guides \(>\) Atlas. Select View \(>\) Stars \(>\) Milky Way to display this galaxy. Select Options \(>\) Stars \(>\) Milky Way, move the Brightness slide-bar to the far right to brighten the Milky Way and click OK. In the View menu, ensure that the Scrollbars are activated and use them to look at different parts of the Milky Way. Can you identify the direction toward the galactic nucleus? In this direction the Milky Way appears broadest. Open the Find pane, enter Sagittarius in the Query box and press Enter to center on this constellation to check your identification. (b) Use this full-sky view to determine the orientation of the plane of the Galaxy with respect to the celestial sphere. Move the vertical scrollbar to its central position to display the Celestial Equator as a horizontal line across the lower part of the view. Move the horizontal scrollbar until the Milky Way is centered upon the view. Estimate the angle between the Milky Way and the celestial equator on the screen. How well aligned is the plane of the Milky Way with the plane of the Earth's equator? (c) A third plane of interest is that of the ecliptic, which is shown as a green line. Use the scrollbars to adjust the view so that the ecliptic appears as a straight line rather than as a curve, thereby ensuring that you are viewing in a direction that lies in the ecliptic plane. Use the horizontal scrollbar to move the view to where you can see where the ecliptic crosses the Milky Way. Estimate the angle between the Milky Way and the ecliptic on the screen. How well aligned is the plane of the Milky Way to the ecliptic, the plane of the Earth's orbit around the Sun? (d) Click on Home in the toolbar to return to your home view, stop Time Flow and set the local time to midnight (12:00:00 A.M.). Select Options > Stars > Milky Way, move the Brightness slide-bar to the far right to brighten the Milky Way and click OK. Adjust the date to January 1, then February 1, and so on. In which month is the galactic nucleus highest in the sky at midnight, so that it is most easily seen from your location?

An RR Lyrae star whose peak luminosity is \(100 \mathrm{~L}_{\odot}\) is in a globular cluster. At its peak luminosity, this star appears from Earth to be only \(1.47 \times 10^{-18}\) as bright as the Sun. Determine the distance to this globular cluster (a) in \(\mathrm{AU}\) and (b) in parsecs.

In what way are the orbits of stars in the galactic disk different from the orbits of planets in our solar system? What does this difference imply about the way that matter is distributed in the Galaxy?

Student book bags often contain a wide collection of oddshaped objects. Each person in your group should rummage through their own book bags and find one object that is most similar to the Milky Way Galaxy in shape. List the items from each group member's belongings and describe what about the items is similar to the shape of our Galaxy and what about the items is not similar, then indicate which of the items is the closest match.

Do density waves form a stationary pattern in a galaxy? If not, do they move more rapidly, less rapidly, or at the same speed as stars in the disk?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free