Logo
Unionpedia
Communication
Get it on Google Play
New! Download Unionpedia on your Android™ device!
Free
Faster access than browser!
 

HR 4102 and Solar luminosity

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between HR 4102 and Solar luminosity

HR 4102 vs. Solar luminosity

I Carinae is a single, yellow-white hued star in the southern constellation Carina. The solar luminosity,, is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.

Similarities between HR 4102 and Solar luminosity

HR 4102 and Solar luminosity have 4 things in common (in Unionpedia): Nuclear fusion, Solar mass, Star, Variable star.

Nuclear fusion

In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons).

HR 4102 and Nuclear fusion · Nuclear fusion and Solar luminosity · See more »

Solar mass

The solar mass is a standard unit of mass in astronomy, equal to approximately.

HR 4102 and Solar mass · Solar luminosity and Solar mass · See more »

Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

HR 4102 and Star · Solar luminosity and Star · See more »

Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.

HR 4102 and Variable star · Solar luminosity and Variable star · See more »

The list above answers the following questions

HR 4102 and Solar luminosity Comparison

HR 4102 has 21 relations, while Solar luminosity has 25. As they have in common 4, the Jaccard index is 8.70% = 4 / (21 + 25).

References

This article shows the relationship between HR 4102 and Solar luminosity. To access each article from which the information was extracted, please visit:

Hey! We are on Facebook now! »