sayyoralar fizikasi

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age23.png ppt/media/image26.png ppt/media/image27.png ppt/media/image28.png ppt/media/image3.png ppt/media/image30.png ppt/media/image31.png ppt/media/image32.png ppt/media/image33.png ppt/media/image34.png ppt/media/image35.png ppt/media/image36.png ppt/media/image37.png ppt/media/image38.png ppt/media/image39.png ppt/media/image4.png ppt/media/image40.png ppt/media/image41.png ppt/media/image42.png ppt/media/image43.png ppt/media/image45.png ppt/media/image46.png ppt/media/image49.png ppt/media/image5.png ppt/media/image50.png ppt/media/image51.png ppt/media/image52.png ppt/media/image53.png ppt/media/image54.png ppt/media/image55.png ppt/media/image57.png ppt/media/image58.png ppt/media/image59.png ppt/media/image6.png ppt/media/image60.png ppt/media/image61.png ppt/media/image63.png ppt/media/image7.png ppt/media/image74.png ppt/media/image75.png ppt/media/image76.png ppt/media/image77.png ppt/media/image8.png ppt/media/image9.png ppt/slides/_rels/slide22.xml.rels ppt/slides/_rels/slide29.xml.rels ppt/slides/slide12.xml ppt/slides/slide14.xml ppt/slides/slide15.xml ppt/slides/slide16.xml ppt/slides/slide18.xml ppt/slides/slide2.xml ppt/slides/slide24.xml ppt/slides/slide25.xml ppt/slides/slide26.xml ppt/slides/slide27.xml ppt/slides/slide28.xml ppt/slides/slide3.xml ppt/slides/slide4.xml ppt/slides/slide40.xml ppt/slides/slide7.xml ppt/slides/slide9.xml [content_types].xml _rels/.rels docprops/custom.xml neptun nomi: neptun quyoshdan uzoqligi : 4 mlrd . 503,4 mln.km diametri : 50100 km zichligi : 1,6 g/sm 3 massasi : 8,6832·10 25 kg o‘z o‘qi atrofida aylanish davri : 17 soat 14 minut quyosh atrofida aylanish davri : 164 yil 280 kun orbital tezligi : 5,4349 km/ sek yo‘ldoshlari : triton, nereida , nayada , talassa , despina , galateya , larissa, … (14 ta). (2018 y.) o‘qining og‘maligi : 97 ,7 7 ° ( teskari aylanadi ) venera qadimgi nomi : zuhro …
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anish davri : 117 yer sutkasi quyosh atrofida aylanish davri : 225 yer sutkasi orbital tezligi : 35 km/ sek yo‘ldoshlari : yo‘q o‘qining og‘maligi : 177 o ( teskari aylanadi ) planetalararo avtomatik stansiya 1974-yilda merkuriydan 47 ming 981 kilometrlik masofadan o‘tayotib , planeta sirtining 500 ga yaqin sifatli rasmlarini oldi . bu rasmlar planeta « yuz tuzilishi » jihatidan oyga juda o‘xshashligini ko‘rsatdi . oy sirtidagi kabi merkuriy yuzasi ham meteoritlar zarbidan « momataloq » bo‘lib , turli kattaliklardagi kraterlar bilan qoplangani , «mariner-10» olgan planeta rasmlaridan shundoqqina ko‘rinib turibdi 9 - mavzu: sayyoralar fizikasi « voyajer»lar yordamida spektroskopik kuzatishlar neptunda vodorod va metan borligini ma’lum qildi . planeta zichligining yupiter va saturn zichligidan ortiqligi , uning tarkibida og‘irroq elementlar mavjud , degan xulosaga olib keldi . yer nomi: yer quyoshdan uzoqligi : 149,6 mln.km diametri : 12756 km zichligi : 5, 5 g/sm 3 massasi : 6 …
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dagi kislorod (0,2%) va suv bug‘idan (0,1%) tashkil topgan . oy osmonining ajoyib hodisalaridan yana biri planetamiz yerning ko‘rinishidir . yer chiroyli , ko‘kimtir shar shaklida , oyning osmondagi ko‘rinishidan to‘rt martacha katta ko‘rinadi . yer ham osmonda oy kabi turli fazalarda ko‘rinadi . bu holat uning quyoshga nisbatan oyning qaysi tomonida turganiga bog‘liq bo‘ladi . yer o‘zining « to‘linyer » fazasida bo‘lganida , oy sirtini to‘linoy yerni yoritgandagidan 40 martacha ravshanroq yoritadi . oy osmonida « to‘linyer » kuzatiladigan payt - yerdan qaraganda oyning yangioy fazasi vaqtiga to‘g‘ri keladi . titsius -bode qoidasi . 1772-yili vittenberglik astronom iogann titsius planetalarning quyoshdan uzoqligini astronomik birliklarda ifodalovchi empirik vositani aniqladi . u quyidagicha : 𝑎 =(0,4 + 0,3 ∗ 2 𝑛 ) 𝑎 . 𝑏 . bu yerda n: -∞, 0, 1, 2, 3, 4, ... qiymatlarni oladi . titsiusning kashfiyotidan xabar topgan berlinlik astronom iogann bode bu empirik munosabatni qayta …

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