Kode Mata Kuliah | AS3104 / 3 SKS |
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Penyelenggara | 103 - Astronomi / FMIPA |
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Kategori | Kuliah |
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| Bahasa Indonesia | English |
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Nama Mata Kuliah | Fisika Bintang | Stellar Physics |
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Bahan Kajian | - Hasil-hasil observasi yang memotivasi berkembangnya studi struktur dan evolusi bintang.
- Atmosfer bintang: proses-proses fisis yang terlibat dan prinsip pemodelannya; contoh solusi model; kaitan antara atmosfer bintang dengan struktur bintang.
- Persamaan struktur bintang dan proses-proses fisis yang terlibat (persamaan keadaan gas, pembangkitan energi, transfer energi).
- Contoh solusi (sederhana) struktur bintang: model politrop dan prediksinya (degenerasi elektron, massa Chandresekhar), dan model lain.
- Pengantar kepada prinsip komputasi struktur dan evolusi bintang tunggal: pembentukan, evolusi bintang tunggal, dan akhir hidup bintang.
- Pengantar (naratif) kepada evolusi bintang ganda berinteraksi.
| - The results of observations that motivated the development of the study of the structure and evolution of stars.
- Star atmosphere: the physical processes involved and the principles of its modeling; examples of model solutions; the relationship between star atmosphere and star structure.
- The star structure equation and the physics processes involved (gas state equation, energy generation, energy transfer)
- Examples of (simple) star structure solutions: politrop models and their predictions (electron degeneration, Chandresekhar masses), and other models.
- Introduction to the computational principles of single star structure and evolution: formation, single star evolution, and the end of star life.
- An introduction (narrative) to the evolution of interacting binary stars.
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Capaian Pembelajaran Mata Kuliah (CPMK) | - Mampu menjelaskan hasil-hasil observasi yang memotivasi berkembangnya studi struktur dan evolusi bintang.
- Mampu menjelaskan proses-proses fisis yang terlibat dalam atmosfer bintang dan prinsip pemodelannya; menunjukkan contoh solusi model; menjelaskan kaitan antara atmosfer bintang dengan struktur bintang.
- Mampu menjelaskan penurunan persamaan struktur bintang dan mengaitkannya dengan proses-proses fisis yang terlibat (persamaan keadaan gas, pembangkitan energi, transfer energi).
- Mampu menjelaskan contoh solusi (sederhana) struktur bintang: model politrop dan prediksinya (degenerasi elektron, massa Chandresekhar), dan model lain.
- Mampu menjelaskan evolusi bintang tunggal: pembentukan, evolusi bintang tunggal, dan akhir hidup bintang.
- Mampu menjelaskan (secara naratif) garis besar evolusi bintang ganda dekat.
| - Able to explain the results of observations that motivate the advanced study of the structure and evolution of stars.
- Able to explain the physics processes involved in the star's atmosphere and the principles of its modeling; showing examples of model solutions; explaining the relationship between star atmospheres and star structures.
- Able to explain the decrease in star structure equations and associate them with the physics processes involved: gas equations, energy generation, energy transfer.
- Able to explain examples of (simple) solutions to star structures: polytropic models and their predictions (electron degeneration, Chandrasekhar masses), and other models.
- Able to explain the evolution of a single star: formation, evolution, and the end of a star's life.
- Able to explain (narratively) the line of evolution of a close binary star.
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Metode Pembelajaran | Kombinasi antara ceramah, diskusi, dan tugas membaca | lectures, discussions, and reading tasks |
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Modalitas Pembelajaran | Sinkron | synchronous |
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Jenis Nilai | ABCDE |
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Metode Penilaian | Kuis, tugas, UTS, UAS | Quiz, Task. Mid-Semester Exam, Final Semester Exam |
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Catatan Tambahan | | |
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