copy and paste this google map to your website or blog!
Press copy button and paste into your blog or website.
(Please switch to 'HTML' mode when posting into your blog. Examples: WordPress Example, Blogger Example)
Star - Wikipedia A star is a luminous spheroid of plasma held together by self-gravity [1] The nearest star to Earth is the Sun Many other stars are visible to the naked eye at night; their immense distances from Earth make them appear as fixed points of light
Star | Definition, Light, Names, Facts | Britannica A star is any massive self-luminous celestial body of gas that shines by radiation derived from its internal energy sources Of the tens of billions of trillions of stars in the observable universe, only a very small percentage are visible to the naked eye
Stars - NASA Science A star’s gas provides its fuel, and its mass determines how rapidly it runs through its supply, with lower-mass stars burning longer, dimmer, and cooler than very massive stars
What Is a Star and How Does It Work? - ThoughtCo How does a star work? How do they form, live, and eventually die? Learn more about these distant objects and their major importance in the universe
What is a Star? Types, Life Cycle, and Fascinating Facts To understand stars is to understand the universe itself This article takes you deep into the heart of stellar science — from the birth of a star in vast clouds of gas and dust, to its dramatic demise as a white dwarf, neutron star, or black hole
What are stars? - BBC Sky at Night Magazine Within each system, the star sits at the centre, providing heat and light that shapes and characterises the planets and other bodies in orbit around it That light may even be the basis for life on some of those worlds, like the Sun in our Solar System
Stars | Astronomy. com This artist’s conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy
Star – Definition Detailed Explanation - Sentinel Mission Main Sequence: The protostar continues to collapse until nuclear fusion begins in its core, leading to the formation of a stable star This stage is known as the main sequence, where the star burns hydrogen into helium
Stars - WorldAtlas As a star approaches the end of its lifespan, it no longer has hydrogen to transform into helium in its core Unable to complete the nuclear fusion process, the star begins to succumb to gravity, slowly collapsing