How do we determine what's in the core of stars/planets?

  • Context: Undergrad 
  • Thread starter Thread starter mace2
  • Start date Start date
  • Tags Tags
    Core
Click For Summary
SUMMARY

Determining the core composition of planets relies heavily on indirect methods, primarily through the study of magnetic fields and seismology. On Earth, seismology has revealed significant insights into the core's structure, while geomagnetic field variations provide additional data on the outer core. For other planets, numerical dynamo models are employed to analyze magnetic field morphology, which can inform us about core properties such as inner core size and convective vigor. Future spacecraft missions are essential for gathering more detailed observations to enhance our understanding of the internal structures of planets like Mercury, Jupiter, Saturn, and Ganymede.

PREREQUISITES
  • Understanding of seismology principles
  • Familiarity with geomagnetic field variations
  • Knowledge of numerical dynamo modeling
  • Basic concepts of planetary magnetic fields
NEXT STEPS
  • Research the application of seismology in planetary science
  • Study geomagnetic field secular variation and its implications
  • Explore numerical dynamo models for planetary cores
  • Investigate upcoming spacecraft missions targeting planetary magnetic fields
USEFUL FOR

Astronomers, planetary scientists, and researchers interested in planetary geology and magnetic field studies will benefit from this discussion.

mace2
Messages
101
Reaction score
0
I tried searching but I must've done something wrong, so...

How do we determine what material is at the core of a planet? Do certain metals emit something we can detect?

I really don't know how to phrase this in an intelligent way, so please bear with me. :biggrin:
 
Astronomy news on Phys.org
Determining properties of a planet's deep interior are difficult because we cannot observe this region directly as we can the surface of a planet. On Earth, seismology has provided important information on the structure and composition of the deep interior including the core. In addition, properties of the Earth's outer core motions have been determined mostly from observations of the geomagnetic field secular variation. Unfortunately we are not at present able to conduct detailed seismic studies and observations of magnetic field secular variation for other planets to provide us with the same quality of information on their cores. We are however, capable of studying a planet's magnetic field morphology quite extensively with an orbiting spacecraft at relatively low altitude. Here we use numerical dynamo models to determine what magnetic field structures can tell us about a planet's core. We concentrate on properties such as inner core size and outer core convective vigor. The results are used to determine what key observations of magnetic field structures could be made by future spacecraft missions to provide information on the dynamo source regions inside planets. This type of study can aid in determining the internal structure and evolution of Mercury, Jupiter, Saturn and Ganymede for which little is known about these properties.

This is an abstract of Determining Core Properties From a Planet's Magnetic Field Morphology
 
So that's how they do it! I never thought of that. Nice abstract though, but I can't get to the full version.
 
Last edited:

Similar threads

  • · Replies 9 ·
Replies
9
Views
4K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 11 ·
Replies
11
Views
3K
  • · Replies 42 ·
2
Replies
42
Views
5K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 148 ·
5
Replies
148
Views
13K
Replies
10
Views
4K
  • · Replies 24 ·
Replies
24
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K