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Eskişehir Academy of Economic and Commercial Sciences, founded in 1958, formed the basis of Anadolu University. The Academy was replaced by Anadolu University in 1982, which has gained a well-deserved place as a modern, dynamic and innovative institution among the largest universities not only in Türkiye, but also in the world.
ACADEMICS
OPEN EDUCATION
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Anadolu University Open Education System plays an essential role in overcoming educational problems of Türkiye not only by providing open and distance education to 1 million active students and 3.5 million graduates but also by developing specific projects. Besides with those numbers, the system is among the mega universities of the world. By the constantly renewing method of open and distance education, it implements many initiatives and innovations in the Turkish Higher Education System.
STUDENT AFFAIRS
RESEARCH
Araştırma
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Kısa adıyla BAP (Bilimsel Araştırma Projeleri), yüksek öğretim kurumlarındaki bilimsel araştırmaların desteklenmesi amacıyla geliştirilmiş bir uygulamadır. Bu uygulama YÖK'ün 01.01.2002 tarihinden geçerli olmak üzere yürülüğe aldığı Yükseköğretim Kurumları Bilimsel Araştırma Projeleri Hakkında Yönetmelik uyarınca gerçekleştirilmektedir. Üniversitemizin tüm öğretim elemanları BAP Komisyonuna başvurarak bilimsel araştırmaları için kaynak alabilirler.
CAMPUS LIFE
Kampüste Yaşam
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At Anadolu University, social and cultural activities are as important as education and scientific research. The University frequently holds scientific events such as conferences, seminars, panels, congresses and symposia, and cultural activities such as exhibitions, stage performances and concerts. In addition to smaller conference halls in each unit, Atatürk Culture and Arts Center, Congress Center and Cinema Anadolu on Yunusemre Campus house many activities throughout the year.

EVOLUTION OF STARS

Content

Weeks	Topics
1. Weeks	Presenting BIRTH OF STARS; Interstellar environment, Gravitation, Stellar formation
2. Weeks	Presenting The Virial Theorem, The Hertzsprung-Russell diagram, Evoluation of stars on the main sequence
3. Weeks	Presenting ADVANCED LEVELS ON STELLAR EVOLUTİON, Evolution of The Sun as the main sequence star
4. Weeks	Presenting After main sequence evolution of small, medium and massive stars
5. Weeks	Presenting Nuclear reactions on stars, Hydrogen flash and red gaint level, Helium flash, Carbon flash.
6. Weeks	Presenting Neon flash, Oxygen flash, Silicon, sulphur and magnesium flash
7. Weeks	Presenting DIED OF STARS, White Dwarfs, Physical formation of White Dwarfs
8. Weeks	Presenting Chandrasekhar limit , Degenerate electron gases, Falling luminosity and internal structure, Collapsing of nuclei and supernovae explosion
9. Weeks	Presenting Classification of supernovae, Physical structure of Nebula, Properties of type II supernovae
10. Weeks	Presenting Properties of type I supernovae , Neutron Stars, Binary pulsar systems
11. Weeks	Presenting Observed rotational rate increase, Physical structure of Neutron Stars, Rotation and magnetic fields of Neutron Stars, Pulsars, Neutron Stars Comparison with Pulsars
12. Weeks	Presenting Producing continuous radiation, The pulsed radiation
13. Weeks	Presenting Black Holes, The Schwarzschild radius
14. Weeks	Presenting Compact X-ray sources, The X-ray production mechanism process