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Related Concept Videos

Globular and Fibrous Proteins02:21

Globular and Fibrous Proteins

Many proteins can be classified into two distinct subtypes - globular or fibrous. These two types differ in their shapes and solubilities.
Globular proteins are also known as spheroproteins and typically are approximately round in shape. They contain a mix of amino acid types and contain differing sequences in their primary structures. Globular proteins have many different functions, such as enzymes, cellular messengers, and molecular transporters. These roles often require the proteins to be...
Globular and Fibrous Proteins02:21

Globular and Fibrous Proteins

Many proteins can be classified into two distinct subtypes - globular or fibrous. These two types differ in their shapes and solubilities.
Globular proteins are also known as spheroproteins and typically are approximately round in shape. They contain a mix of amino acid types and contain differing sequences in their primary structures. Globular proteins have many different functions, such as enzymes, cellular messengers, and molecular transporters. These roles often require the proteins to be...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Globular Proteins01:27

Globular Proteins

In organisms, proteins are the most abundant macromolecules. They act as the building blocks of life and play various crucial roles in the body. Proteins can be broadly classified into two distinct subtypes based on their shape and solubilities: globular proteins and fibrous proteins.
Globular proteins serve many important physiological functions, such as acting as enzymes, cellular messengers, and molecular transporters. These roles often require the proteins to be soluble in the aqueous...
Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.

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Related Experiment Video

Updated: Jun 1, 2026

Studying Organelle Dynamics in B Cells During Immune Synapse Formation
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Studying Organelle Dynamics in B Cells During Immune Synapse Formation

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A black hole in a globular cluster.

Thomas J Maccarone1, Arunav Kundu, Stephen E Zepf

  • 1School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK. tjm@phys.soton.ac.uk

Nature
|January 5, 2007
PubMed
Summary

Astronomers detected an accreting black hole in a globular cluster within galaxy NGC 4472. This finding provides evidence for black hole formation and survival in dense stellar environments.

Area of Science:

  • Astrophysics
  • Stellar Dynamics
  • X-ray Astronomy

Background:

  • Globular clusters are dense collections of old stars.
  • High stellar densities suggest frequent stellar interactions and collisions.
  • The existence of black holes within globular clusters is debated due to theoretical predictions of their formation and ejection.

Purpose of the Study:

  • To investigate the presence of black holes in globular clusters.
  • To provide observational evidence for black hole formation and survival in these dense stellar systems.

Main Methods:

  • X-ray observations of a globular cluster in the giant elliptical galaxy NGC 4472.
  • Analysis of X-ray luminosity and variability to identify the nature of the compact object.

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Main Results:

  • Detection of an accreting object with an X-ray luminosity of approximately 4 x 10^39 erg s^-1.
  • The object's luminosity is consistent with a black hole in an old stellar population.
  • Rapid X-ray luminosity variations (factor of seven in a few hours) rule out superposition of neutron stars.

Conclusions:

  • The observed X-ray signature strongly indicates the presence of an accreting black hole within the globular cluster.
  • This discovery supports theories suggesting black holes can form and persist in the dense environments of globular clusters.
  • The findings contribute to understanding the end-states of stellar evolution and compact object populations in dense stellar systems.