Apparent Magnitude: Meaning & 3 Star System

Click For Summary
SUMMARY

The apparent magnitude of a star quantifies its brightness as observed from Earth, utilizing a logarithmic scale where 0 represents the brightest stars, 6 is the limit of human visibility, and 26 is the threshold for large telescopes. The discussion clarifies that the "system of 3 stars" likely refers to comparing an unknown star's brightness to three known stars, possibly in reference to the Delta Cephei experiment. The magnitude scale is not linear; for instance, three stars with an apparent magnitude of 3 collectively appear as bright as a single star with a magnitude of 1.8. To calculate combined brightness, individual magnitudes must be converted to luminosity, summed, and then converted back to magnitude.

PREREQUISITES
  • Understanding of logarithmic scales in astronomy
  • Familiarity with the concept of luminosity
  • Knowledge of the Delta Cephei experiment
  • Basic principles of stellar brightness and distance
NEXT STEPS
  • Research the Delta Cephei experiment and its significance in measuring stellar brightness
  • Learn about the conversion process between apparent magnitude and luminosity
  • Explore the historical context of Hipparchus and the development of the magnitude scale
  • Investigate the differences between apparent magnitude and absolute magnitude
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in understanding stellar brightness and measurement techniques.

Magister
Messages
82
Reaction score
0
What is the meaning of: "the apparent magnitude of a star is obtain with a system of 3 stars"?

Thanks
 
Astronomy news on Phys.org
"apparent magnitude" is how bright a star looks from earth.
It's on a rather odd log scale from 0=brightest, 6 is the about the limit with your eye, 26 is about the record for a big telescope.

Not sure about the "system of 3 stars" could mean either that you compare the unknown star with 3 known stars nearby ( is this the delta cephei experiment) .
The star Vega used to be defined as magnitude 0 but then you just use each magnitude being 2.5 times fainter than the previous - there is no standard mag=1,2,3 etc star.
 
Sounds live an equivalent single star brightness question. The magnitude scale is logarithmic, so magnitudes do not multiply of divide linearly. For example 3 stars of apparent magnitude 3 would collectively appear about as bright as one star of apparent magnitude 1.8. The most straightforward way to obtain combined brightness of individual stars is to convert each individual magnitudes to luminosity, add them up and then convert back to magnitude.
 
"Apparent magnitude" is a kind of brightness quantity. But as you guess, brightness depends on the distance between observer and a object. Apparent magnitude is just the brightness, when you observe it from the Earth with, or from space telescope from space. But be careful, its unit is not just the same with brightness(whose is energy/time). After Hipparchus, who was the first sky watcher to determine the locations of the stars, and he also labeled the brightest star as 1 magnitude, and the faintest with 6 magnitude.
 

Similar threads

  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 8 ·
Replies
8
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
5
Views
2K
  • · Replies 14 ·
Replies
14
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 6 ·
Replies
6
Views
3K