找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Introduction to Astronomy and Astrophysics; Arnold Hanslmeier Textbook 20231st edition Springer-Verlag GmbH Germany, part of Springer Natu

[復(fù)制鏈接]
樓主: gloomy
21#
發(fā)表于 2025-3-25 04:15:20 | 只看該作者
22#
發(fā)表于 2025-3-25 08:55:43 | 只看該作者
978-3-662-64639-7Springer-Verlag GmbH Germany, part of Springer Nature 2023
23#
發(fā)表于 2025-3-25 14:55:15 | 只看該作者
History of Astronomy,In this section we give an overview of the history of astronomy.
24#
發(fā)表于 2025-3-25 19:29:46 | 只看該作者
Celestial Mechanics,The centuries after Newton were the heyday of celestial mechanics. At first it was about the description of the planetary orbits, soon followed by precise orbital calculations. In 1682,. observed the comet that was later named after him. The last apparition was 1985/1986.
25#
發(fā)表于 2025-3-25 23:58:09 | 只看該作者
Astronomical Instruments,Before the light of astronomical objects reaches the Earth’s surface and thus the telescope of an observatory or the receiver (CCD, photoplate, eye), it is exposed to numerous changes:
26#
發(fā)表于 2025-3-26 04:07:32 | 只看該作者
The Sun,Our Sun is the only star whose surface we can study in detail due to its proximity. Through space missions are also . measurements possible.
27#
發(fā)表于 2025-3-26 05:04:20 | 只看該作者
State Variables of Stars,In this section we discuss the determination of the most important properties or state variables of a star: radius, temperature, mass, density, gravitational acceleration, chemical composition, magnetic field as well as rotation. First, we briefly review the trigonometric distance determination.
28#
發(fā)表于 2025-3-26 10:15:53 | 只看該作者
Stellar Atmospheres,The term stellar atmosphere is very broad: In principle, it is understood to mean those layers of a star in which the spectral lines are formed. In our . this essentially occurs in the . (only 400 km thick) but also in Chromosphere and even in the Corona.
29#
發(fā)表于 2025-3-26 13:29:30 | 只看該作者
Stellar Structure,In this chapter we cover the main equations describing the structure of a star. Furthermore, we trace the evolution of stars in the Hertzsprung-Russell diagram.
30#
發(fā)表于 2025-3-26 18:38:42 | 只看該作者
Stellar Evolution,In principle, there are the following stages in stellar evolution:
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2026-1-21 22:57
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
德兴市| 和田县| 衡山县| 吴堡县| 龙口市| 内江市| 乌拉特后旗| 河南省| 长葛市| 福安市| 和平县| 正定县| 苏尼特左旗| 安康市| 孟村| 富平县| 嘉荫县| 濮阳县| 始兴县| 灵台县| 冀州市| 江西省| 德兴市| 万载县| 鲁山县| 六枝特区| 白城市| 如皋市| 嵊州市| 金乡县| 什邡市| 小金县| 佛坪县| 庄浪县| 三台县| 永胜县| 洪泽县| 左云县| 罗源县| 中阳县| 祁门县|