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地球科學 1941

《日射準則與冰期問題》

米盧廷·米蘭科維奇

地球軌道的緩慢擺動調暗了高緯度的夏日陽光——並為冰期定下節拍。

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In depth · the introduction

冰期的來去並非隨機——它們與地球在軌道上的緩慢搖擺同步而行。

核心思想

地球繞日的方式並非一成不變。它的軌道時而拉長、時而復圓;它的地軸時而更直立些、時而更傾斜些;而那傾斜的地軸又像陀螺般緩緩打轉,改變著「地球離太陽最近時正逢哪個季節」。每一種擺動都很輕微,又各以漫長的節律重複——動輒數萬年。

米盧廷·米蘭科維奇證明:它們合在一起,會改變到達遙遠北方的夏季陽光有多少。而要緊的,正是那裡的夏季太陽:當北方的夏天變涼,前一個冬天的積雪便無法完全融盡。年復一年,雪越積越厚,冰期於是開始。暖夏把雪融退,冰川便後撤。

它如何形成

這一想法有位蘇格蘭先驅——自學成才、當過門房的科學家詹姆斯·克羅爾(James Croll)。他在 1860 年代把冰期與軌道聯繫起來——卻錯猜成因是寒冷的冬天。米蘭科維奇,一位轉任貝爾格萊德教授的塞爾維亞工程師,約從 1911 年起立志把整件事化為精確的數學,地球、火星、金星一併算來。

那是一生的手算。第一次世界大戰期間,他甚至以戰俘之身,在布達佩斯的一座圖書館裡繼續演算。關鍵的指點來自氣候學家弗拉迪米爾·柯本(Wladimir Köppen)——他與女婿、以「大陸漂移」聞名的阿爾弗雷德·韋格納一道,勸米蘭科維奇聚焦於高緯度的夏季。他們 1924 年的著作刊出了米蘭科維奇的曲線,而它與已知的四次阿爾卑斯冰期一一吻合。

它為何重要

冰期第一次有了一座鐘。不再是「過去比較冷」這樣含糊的故事,而是寫在太陽系幾何裡的、對冰川何時進退的精確預言。它把我們這顆行星的氣候史,繫到了諸天的運動之上,也給了地質學家一份可與岩石——並最終與海底的泥芯——對照檢驗的曆法。

一個類比

想象有三個調光開關,接在照向遙遠北方的夏季太陽上。一個是地球的傾角,一個是軌道的形狀,一個是季節的時機。每個都按自己緩慢的時間表上下滑動。多數時候,它們的設置彼此部分抵消。但每隔一陣,三者會一齊調暗——北方的夏天變得黯淡而涼爽,雪不再融化,冰便向南爬行。米蘭科維奇的成就,正是把這三個旋鈕的確切位置,一讀就讀了幾十萬年。

一個傾斜的地球、一個太陽位於焦點的小軌道,以及一個北緯 65° 夏季陽光的豎直量表。三個滑桿設定傾角、軌道形狀與夏季落點;移動它們,量表隨之變亮或變暗。

它的位置

米蘭科維奇糾正並補全了一個比他更古老的想法(阿德馬爾、克羅爾),又把它交給了未來。它在整個 1950 年代被否定,卻在 1976 年獲得證實——人們發現深海岩芯恰恰以他那些軌道週期脈動。如今,它支撐著我們為地球史最近這幾百萬年的定年。它屬於本館其他幾把氣候之鑰——阿倫尼烏斯論溫室效應(arrhenius-1896)、基林所測上升的二氧化碳(keeling-1960)——也與韋格納漂移的大陸(wegener-1912)為伴:正是韋格納的合作者柯本,幫米蘭科維奇指對了方向。

The original document
Original source text
Milutin Milanković (1879–1958) · Kanon der Erdbestrahlung und seine Anwendung auf das Eiszeitenproblem · Royal Serbian Academy, Belgrade, 1941 (in German)
The cosmic problem
Milanković opens by setting himself a single, audacious problem: to compute, from celestial mechanics alone, exactly how much solar radiation each latitude of a planet receives in each season — and how that has changed over geological time. He solves it for the Earth and sketches it for Mars and Venus. The whole edifice rests on Newtonian gravitation and spherical astronomy; nothing is fitted to the geological record in advance.
The three orbital elements
Three slow changes in the Earth's motion govern the answer. The eccentricity of the orbit — how far from a circle the ellipse is — breathes in and out over roughly 100,000 and 413,000 years. The obliquity, the tilt of the spin axis, nods between about 22.1° and 24.5° over roughly 41,000 years. And the precession of the equinoxes — the slow swivel of the tilted axis, combined with the turning of the orbit's own long axis — shifts the season at which the Earth is nearest the Sun, with periods near 23,000 and 19,000 years.
The insolation integral
From these elements Milanković integrates the radiation arriving over a day and over a 'caloric' half-year. With Köppen's advice he fixes attention on the summer half-year at high northern latitudes, expressing each result as the latitude that would receive the same summer radiation today — the 65°N equivalent latitude. The governing quantity is the high-latitude summer insolation, not the annual total.
The curves of the past 600,000 years
He computes the summer-insolation curve back through six hundred millennia, entirely by hand. The criterion, again Köppen's: ice ages are born of cool summers that fail to melt the winter snow, not of cold winters. The dips in the curve are read as glacial epochs — and they line up with the four Alpine glaciations (Günz, Mindel, Riss, Würm) that Penck and Brückner had mapped from the field.
What lies beyond the astronomy
Milanković is candid that the orbital forcing is only the trigger. The amplification — growing ice that reflects more sunlight, shifting oceans and carbon — belongs to a physics he does not claim to have solved. The Canon supplies the metronome; the orchestra of feedbacks is left to others.
[ … ]
Belgrade, 1941