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Kanbun-LM is not shown here because automatic generation is Japanese-only. This patch keeps the manual path as the default workflow.

Source page


# WORK_TITLE: 恆星
# DISPLAY_TITLE: 恆星
# AUTHOR:
# TIMES:
# PAGE_TITLE: 恆星
# CATEGORIES:
昴宿，實
疏散星團
也

恆星
者，天上星體也，一名
列星，亦名
經星，恆者謂其象終古不易也
（然實有易，惟於吾人而言，微之又微而已）。蓋其實為
等離子體
（吾人所知物有三態︰曰固、曰液、曰氣，然三態之外，實尚有等離子態）。巨且生光。世人仰天所望者，所以為星者，多是。吾人所煗者
日，亦所屬。日近而他星遠，故日照時，諸星幽暗，俟日落後，方能目之。

自古以還，無所知其實為何物。及至當世，泰西
格致
彊甚，方知其內多為
氫
氦
二氣，經
核融合
化氫為氦。能量遂生，越萬里而至
地球，吾人方目之矣
（能量為泰西詞，蓋光、電、力、勢皆其屬也）。

經其
光譜、
亮度、動向，可斷其質、歲及
化學
成份
（化學，泰西格物致知之學，所以觀萬物所遷化也；成份，合成之方也，亦為泰西詞）。

蓋其伊始，天氣凝聚，無知其由。氫化為氦，積于其中。其中心氫盡，內遂虛，歷千萬億年而崩，或為
黑洞、或為
中子星、或為
白矮星
（此皆其亡後之狀，亡前先脹，曰紅巨星，爾後或爆，其狀曰超新星；諸詞悉為泰西所創，其意甚艱，詳見內文，兹不贅）。
宇宙浩渺， 然星多非生而獨處，亦有互制互生者，曰
雙星
。亦有叢聚而生者，其名則定以星之多寡。星寡者曰
聚星，多者曰
星團
。
（多以百為界，數十者為聚星，又疏星團有星數千，簇星團可達百萬餘。）據

湯若望《新法表異》

《天文學新概論》

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Punctuation options

Preset Source Modern CJK (Traditional) Modern CJK (Simplified / PRC) Pure classical Strip Custom

Quotes

Family

Chinese quotation marks 「」『』 Latin speech marks “ ” ‘ ’ Chinese speech marks ＂＇ Off

Ordering

Traditional: 「甲『乙』丙」 Simplified: 『甲「乙」丙』 Vertical quote forms (﹁﹂﹃﹄)

Question / Exclamation Keep ？ Collapse ? → 。

Keep ！ Collapse ! → 。

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Comma Use ， Use 、

Repetition mark No repetition mark (default) 々 (Horizontal) 〻 (Vertical) 二 (Western Zhou-style)

# WORK_TITLE: 恆星 # DISPLAY_TITLE: 恆星 # AUTHOR: # TIMES: # PAGE_TITLE: 恆星 # CATEGORIES: 昴宿，實疏散星團也恆星者，天上星體也，一名列星，亦名經星，恆者謂其象終古不易也（然實有易，惟於吾人而言，微之又微而已）。蓋其實為等離子體（吾人所知物有三態︰曰固、曰液、曰氣，然三態之外，實尚有等離子態）。巨且生光。世人仰天所望者，所以為星者，多是。吾人所煗者日，亦所屬。日近而他星遠，故日照時，諸星幽暗，俟日落後，方能目之。自古以還，無所知其實為何物。及至當世，泰西格致彊甚，方知其內多為氫氦二氣，經核融合化氫為氦。能量遂生，越萬里而至地球，吾人方目之矣（能量為泰西詞，蓋光、電、力、勢皆其屬也）。經其光譜、亮度、動向，可斷其質、歲及化學成份（化學，泰西格物致知之學，所以觀萬物所遷化也；成份，合成之方也，亦為泰西詞）。蓋其伊始，天氣凝聚，無知其由。氫化為氦，積于其中。其中心氫盡，內遂虛，歷千萬億年而崩，或為黑洞、或為中子星、或為白矮星（此皆其亡後之狀，亡前先脹，曰紅巨星，爾後或爆，其狀曰超新星；諸詞悉為泰西所創，其意甚艱，詳見內文，兹不贅）。宇宙浩渺，然星多非生而獨處，亦有互制互生者，曰雙星。亦有叢聚而生者，其名則定以星之多寡。星寡者曰聚星，多者曰星團。（多以百為界，數十者為聚星，又疏星團有星數千，簇星團可達百萬餘。）據湯若望《新法表異》《天文學新概論》