A Short History of Nearly Everything萬物簡史 英文原版 [平裝] pdf epub mobi txt 電子書 下載 2025

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☆☆☆☆☆

Bill Bryson（比爾·布萊森） 著

圖書標籤:

• 科學
• 曆史
• 科普
• 非虛構
• 物理
• 化學
• 生物
• 宇宙
• 地球
• 知識

齣版社： Broadway Books

ISBN：9780767908184

商品編碼：19463061

包裝：平裝

齣版時間：2004-09-14

用紙：膠版紙

頁數：544

正文語種：英文

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　　這是一部有關現代科學發展史的既通俗易懂又引人入勝的書，作者用清晰明瞭、幽默風趣的筆法，將宇宙大爆炸到人類文明發展進程中所發生的繁多妙趣橫生的故事一一收入筆下。驚奇和感嘆組成瞭這本書，曆曆在目的天下萬物組成瞭這本書，益於人們瞭解大韆世界的無窮奧妙，掌握萬事萬物的發展脈絡。本書2003年5月在美國齣版後，連續數十周高居《紐約時報》、《泰晤士報》排行榜最前列，在年度科學圖書排行榜中，本書更是勇奪桂冠！

內容簡介

One of the world’s most beloved writers and bestselling author of One Summer takes his ultimate journey—into the most intriguing and intractable questions that science seeks to answer.

In A Walk in the Woods, Bill Bryson trekked the Appalachian Trail—well, most of it. In A Sunburned Country, he confronted some of the most lethal wildlife Australia has to offer. Now, in his biggest book, he confronts his greatest challenge: to understand—and, if possible, answer—the oldest, biggest questions we have posed about the universe and ourselves. Taking as territory everything from the Big Bang to the rise of civilization, Bryson seeks to understand how we got from there being nothing at all to there being us. To that end, he has attached himself to a host of the world’s most advanced (and often obsessed) archaeologists, anthropologists, and mathematicians, travelling to their offices, laboratories, and field camps. He has read (or tried to read) their books, pestered them with questions, apprenticed himself to their powerful minds. A Short History of Nearly Everything is the record of this quest, and it is a sometimes profound, sometimes funny, and always supremely clear and entertaining adventure in the realms of human knowledge, as only Bill Bryson can render it. Science has never been more involving or entertaining.

　　這是一部有關現代科學發展史的既通俗易懂又引人入勝的書，作者用清晰明瞭、幽默風趣的筆法，將宇宙大爆炸到人類文明發展進程中所發生的繁多妙趣橫生的故事一一收入筆下。驚奇和感嘆組成瞭本書，曆曆在目的天下萬物組成瞭本書，益於人們瞭解大韆世界的無窮奧妙，掌握萬事萬物的發展脈絡。
　　書中迴溯瞭科學史上那些偉大與奇妙的時刻，引用瞭近年來發現的最新科學史料，幾乎每一個被作者描述的事件都奇特而且驚人：宇宙起源於一個要用顯微鏡纔能看得見的奇點；全球氣候變暖可能會使北美洲和歐洲北部地區變得更加寒冷；1815年印度尼西亞鬆巴哇島坦博士拉火山噴發，噴湧而齣的熔岩以及相伴而來的海嘯奪走瞭10萬人的生命；美國黃石國傢公園是“世界上最大的活火山”……而那些沉迷於科學的科學傢們也是韆奇百怪：達爾文居然為蚯蚓彈起瞭鋼琴；牛頓將一根大針眼縫針插進眼窩，為的隻是看看會有什麼事情發生；富蘭剋林不顧生命危險在大雷雨裏放風箏；卡文迪許在自己身上做電擊強度實驗，竟然到瞭失去知覺的地步……
　　本書在講述科學的奇跡與成就的同時，還浸潤著濃鬱的悲天憫人的人文關懷。全書從科學發展史的角度對“我們從哪裏來？我們是誰？我們到哪裏去？”這一韆古命題作瞭極為精當的闡釋，每一個人在閱讀此書之後，都會對生命、對人生、對我們所生活的世界産生全新的感悟。一位美國小讀者的父親說，讀過《萬物簡史》之後，他對死亡不再感到恐懼……作者認為，這是一本書所能獲得的最高評價。

作者簡介

Bill Bryson was born in Des Moines, Iowa. For twenty years he lived in England, where he worked for the Times and the Independent, and wrote for most major British and American publications. His books include travel memoirs (Neither Here Nor There; The Lost Continent; Notes from a Small Island) and books on language (The Mother Tongue; Made in America). His account of his attempts to walk the Appalachian Trail, A Walk in the Woods, was a huge New York Times bestseller. He lives in Hanover, New Hampshire, with his wife and his four children.

　　比爾·布萊森，享譽世界的旅遊文學作傢。1951年齣生於美國艾奧瓦州，畢業於美國德雷剋大學。從1973年起，曾在英國居住20年之久，任職於《泰晤士報》與《獨立報》，同時也為《紐約時報》、《國傢地理雜誌》等刊物撰文。後搬迴美國，現與妻子和四個小孩居住於新罕布什爾州的漢諾威市。
　　布萊森擅長用不同的眼光來看待他所遊曆的世界，在他的書裏，英國式的睿智幽默與美國式的搞笑絕妙地融閤在瞭一起。他的尖刻加上他的博學，讓他的文字充滿瞭幽默、機敏和智慧，使他自己成為“目前活在世上的最有趣的旅遊文學作傢”（《泰晤士報》）。
　　代錶作有《哈！小不列顛》、《歐洲在發酵》、《一腳踩進小美國》、《彆跟山過不去》、《請問這裏是美國嗎？》等多種，每本均高居美、英、加暢銷書排行榜前列。其中《哈！小不列顛》更被英國讀者推選為“最能深刻傳達齣英國靈魂的作品”。
　　作者不但纔華橫溢，興趣亦十分廣泛，在語言學方麵著有《麻煩詞匯詞典》、《母語》、《美式英語》等書，皆為擁有廣大擁躉的幽默之作。

精彩書評

"Stylish [and] stunningly accurate prose. We learn what the material world is like from the smallest quark to the largest galaxy and at all the levels in between . . . brims with strange and amazing facts . . . destined to become a modern classic of science writing."
--The New York Times

"Bryson has made a career writing hilarious travelogues, and in many ways his latest is more of the same, except that this time Bryson hikes through the world of science."
--People

"Bryson is surprisingly precise, brilliantly eccentric and nicely eloquent . . . a gifted storyteller has dared to retell the world's biggest story."
--Seattle Times

"Hefty, highly researched and eminently readable."
--Simon Winchester, The Globe and Mail

"All non-scientists (and probably many specialized scientists, too) can learn a great deal from his lucid and amiable explanations."
--National Post

"Bryson is a terrific stylist. You can't help but enjoy his writing, for its cheer and buoyancy, and for the frequent demonstration of his peculiar, engaging turn of mind."
--Ottawa Citizen

"Wonderfully readable. It is, in the best sense, learned."
--Winnipeg Free Press

前言/序言

1 HOW TO BUILD A UNIVERSE
NO MATTER HOW hard you try you will never be able to grasp just how tiny, how spatially unassuming, is a proton. It is just way too small.
A proton is an infinitesimal part of an atom, which is itself of course an insubstantial thing. Protons are so small that a little dib of ink like the dot on this i can hold something in the region of 500,000,000,000 of them, rather more than the number of seconds contained in half a million years. So protons are exceedingly microscopic, to say the very least.
Now imagine if you can (and of course you can't) shrinking one of those protons down to a billionth of its normal size into a space so small that it would make a proton look enormous. Now pack into that tiny, tiny space about an ounce of matter. Excellent. You are ready to start a universe.
I'm assuming of course that you wish to build an inflationary universe. If you'd prefer instead to build a more old-fashioned, standard Big Bang universe, you'll need additional materials. In fact, you will need to gather up everything there is--every last mote and particle of matter between here and the edge of creation--and squeeze it into a spot so infinitesimally compact that it has no dimensions at all. It is known as a singularity.
In either case, get ready for a really big bang. Naturally, you will wish to retire to a safe place to observe the spectacle. Unfortunately, there is nowhere to retire to because outside the singularity there is no where. When the universe begins to expand, it won't be spreading out to fill a larger emptiness. The only space that exists is the space it creates as it goes.
It is natural but wrong to visualize the singularity as a kind of pregnant dot hanging in a dark, boundless void. But there is no space, no darkness. The singularity has no "around" around it. There is no space for it to occupy, no place for it to be. We can't even ask how long it has been there--whether it has just lately popped into being, like a good idea, or whether it has been there forever, quietly awaiting the right moment. Time doesn't exist. There is no past for it to emerge from.
And so, from nothing, our universe begins.
In a single blinding pulse, a moment of glory much too swift and expansive for any form of words, the singularity assumes heavenly dimensions, space beyond conception. In the first lively second (a second that many cosmologists will devote careers to shaving into ever-finer wafers) is produced gravity and the other forces that govern physics. In less than a minute the universe is a million billion miles across and growing fast. There is a lot of heat now, ten billion degrees of it, enough to begin the nuclear reactions that create the lighter elements--principally hydrogen and helium, with a dash (about one atom in a hundred million) of lithium. In three minutes, 98 percent of all the matter there is or will ever be has been produced. We have a universe. It is a place of the most wondrous and gratifying possibility, and beautiful, too. And it was all done in about the time it takes to make a sandwich.
When this moment happened is a matter of some debate. Cosmologists have long argued over whether the moment of creation was 10 billion years ago or twice that or something in between. The consensus seems to be heading for a figure of about 13.7 billion years, but these things are notoriously difficult to measure, as we shall see further on. All that can really be said is that at some indeterminate point in the very distant past, for reasons unknown, there came the moment known to science as t = 0. We were on our way.
There is of course a great deal we don't know, and much of what we think we know we haven't known, or thought we've known, for long. Even the notion of the Big Bang is quite a recent one. The idea had been kicking around since the 1920s, when Georges Lem tre, a Belgian priest-scholar, first tentatively proposed it, but it didn't really become an active notion in cosmology until the mid-1960s when two young radio astronomers made an extraordinary and inadvertent discovery.
Their names were Arno Penzias and Robert Wilson. In 1965, they were trying to make use of a large communications antenna owned by Bell Laboratories at Holmdel, New Jersey, but they were troubled by a persistent background noise--a steady, steamy hiss that made any experimental work impossible. The noise was unrelenting and unfocused. It came from every point in the sky, day and night, through every season. For a year the young astronomers did everything they could think of to track down and eliminate the noise. They tested every electrical system. They rebuilt instruments, checked circuits, wiggled wires, dusted plugs. They climbed into the dish and placed duct tape over every seam and rivet. They climbed back into the dish with brooms and scrubbing brushes and carefully swept it clean of what they referred to in a later paper as "white dielectric material," or what is known more commonly as bird shit. Nothing they tried worked.
Unknown to them, just thirty miles away at Princeton University, a team of scientists led by Robert Dicke was working on how to find the very thing they were trying so diligently to get rid of. The Princeton researchers were pursuing an idea that had been suggested in the 1940s by the Russian-born astrophysicist George Gamow that if you looked deep enough into space you should find some cosmic background radiation left over from the Big Bang. Gamow calculated that by the time it crossed the vastness of the cosmos, the radiation would reach Earth in the form of microwaves. In a more recent paper he had even suggested an instrument that might do the job: the Bell antenna at Holmdel. Unfortunately, neither Penzias and Wilson, nor any of the Princeton team, had read Gamow's paper.
The noise that Penzias and Wilson were hearing was, of course, the noise that Gamow had postulated. They had found the edge of the universe, or at least the visible part of it, 90 billion trillion miles away. They were "seeing" the first photons--the most ancient light in the universe--though time and distance had converted them to microwaves, just as Gamow had predicted. In his book The Inflationary Universe, Alan Guth provides an analogy that helps to put this finding in perspective. If you think of peering into the depths of the universe as like looking down from the hundredth floor of the Empire State Building (with the hundredth floor representing now and street level representing the moment of the Big Bang), at the time of Wilson and Penzias's discovery the most distant galaxies anyone had ever detected were on about the sixtieth floor, and the most distant things--quasars--were on about the twentieth. Penzias and Wilson's finding pushed our acquaintance with the visible universe to within half an inch of the sidewalk.
Still unaware of what caused the noise, Wilson and Penzias phoned Dicke at Princeton and described their problem to him in the hope that he might suggest a solution. Dicke realized at once what the two young men had found. "Well, boys, we've just been scooped," he told his colleagues as he hung up the phone.
Soon afterward the Astrophysical Journal published two articles: one by Penzias and Wilson describing their experience with the hiss, the other by Dicke's team explaining its nature. Although Penzias and Wilson had not been looking for cosmic background radiation, didn't know what it was when they had found it, and hadn't described or interpreted its character in any paper, they received the 1978 Nobel Prize in physics. The Princeton researchers got only sympathy. According to Dennis Overbye in Lonely Hearts of the Cosmos, neither Penzias nor Wilson altogether understood the significance of what they had found until they read about it in the New York Times.
Incidentally, disturbance from cosmic background radiation is something we have all experienced. Tune your television to any channel it doesn't receive, and about 1 percent of the dancing static you see is accounted for by this ancient remnant of the Big Bang. The next time you complain that there is nothing on, remember that you can always watch the birth of the universe.
Although everyone calls it the Big Bang, many books caution us not to think of it as an explosion in the conventional sense. It was, rather, a vast, sudden expansion on a whopping scale. So what caused it?
One notion is that perhaps the singularity was the relic of an earlier, collapsed universe--that we're just one of an eternal cycle of expanding and collapsing universes, like the bladder on an oxygen machine. Others attribute the Big Bang to what they call "a false vacuum" or "a scalar field" or "vacuum energy"--some quality or thing, at any rate, that introduced a measure of instability into the nothingness that was. It seems impossible that you could get something from nothing, but the fact that once there was nothing and now there is a universe is evident proof that you can. It may be that our universe is merely part of many larger universes, some in different dimensions, and that Big Bangs are going on all the time all over the place. Or it may be that space and time had some other forms altogether before the Big Bang--forms too alien for us to imagine--and that the Big Bang represents some sort of transition phase, where the universe went from a form we can't understand to one we almost can. "These are very close to religious questions," Dr. Andrei Linde, a cosmologist at Stanford, told the New York Times in 2001.
The Big Bang theory isn't about the bang itself but about what happened after the bang. Not long after, mind you. By doing a lot of math and watching carefully what goes on in particle accelerators, scientists believe they can look back to 10-43 seconds after the moment of creation, when the universe was still so small that you would have needed a microscope to find it. We mustn't swoon over every extraordinary number that comes before us, but it is perhaps worth l...

《宇宙的奇妙旅程：從大爆炸到人類文明的宏偉敘事》 一部探索時間、空間、生命與我們自身起源的史詩級著作 作者：[虛構作者姓名] 譯者：[虛構譯者姓名] 齣版社：[虛構齣版社名稱] --- 內容概要： 《宇宙的奇妙旅程》並非僅僅是一部科學史的編年史，它是一次橫跨近140億年時空的深度潛航，旨在迴答人類最根本的哲學追問：我們從哪裏來？宇宙如何演化至此？生命如何在看似不可能的環境中勃發？以及，我們作為智慧的産物，在浩瀚的宇宙圖景中占據何種位置？ 本書以宏大敘事的手法，將物理學、化學、地質學、生物學、古人類學和天文學的知識熔於一爐，構建瞭一個連貫、引人入勝的知識體係。作者摒棄瞭晦澀難懂的專業術語，以清晰、富有洞察力的筆觸，帶領讀者體驗科學發現的激動人心時刻，理解那些徹底改變人類世界觀的關鍵轉摺點。 第一部分：無中生有——宇宙的黎明與物質的誕生 本部分深入探討宇宙的開端——那個被稱為“奇點”的瞬間，以及隨後發生的暴脹時代。我們追溯瞭物理學定律的形成過程，解釋瞭為什麼宇宙的基本常數恰好允許物質的存在。從誇剋到質子、中子，再到宇宙微波背景輻射的形成，作者詳細描繪瞭宇宙“黑暗時期”的圖景，以及第一代恒星如何點燃瞭宇宙的燈火。 重點關注恒星的生命周期及其在元素煉金術中的作用。我們學習到，構成我們身體的碳、氧、鐵等重元素，並非宇宙之初就已存在，而是來自超新星爆炸的壯烈謝幕。這部分將物質的起源與宇宙的命運緊密聯係起來，揭示瞭我們與遙遠星辰之間血脈相連的深刻事實。 第二部分：地球的塑型——行星的形成與生命的萌芽 當我們把目光聚焦到銀河係的一個不起眼的鏇臂上時，本書進入瞭太陽係的形成階段。作者細緻地重建瞭原始太陽星雲的演化過程，解釋瞭行星如何通過吸積作用凝聚成型。隨後，敘事轉嚮地球——這顆獨特的藍色行星。 地質學成為主綫，描述瞭地球內部的構造活動、闆塊漂移的漫長舞蹈，以及磁場如何為生命的誕生創造瞭必要的保護層。本書對“原始湯”理論進行瞭深入探討，分析瞭地球早期海洋環境中，無機物如何通過化學反應，偶然卻必然地形成瞭第一個能夠自我復製的分子。化學的魔力在這裏達到瞭頂峰，我們見證瞭生命（生命體）的第一個微小、脆弱的細胞前體的齣現。 第三部分：進化的狂想麯——從單細胞到物種大爆炸 生命齣現之後，其演化之路充滿瞭偶然與必然的交織。本部分聚焦於生物學革命性的裏程碑。從原核生物到真核生物的飛躍，從有性生殖的齣現到寒武紀“生命大爆炸”的奇觀，作者係統地梳理瞭生命形式的復雜性是如何逐步增加的。 尤其引人注目的是對關鍵進化事件的生動再現：植物登陸如何重塑大氣成分，昆蟲的翅膀如何開啓瞭天空的徵服，以及脊椎動物如何從水中走嚮陸地。書中詳細剖析瞭諸如大規模滅絕事件（如二疊紀-三疊紀的“大死亡”和白堊紀-古近紀的撞擊事件）對生命多樣性格局的深遠影響，並強調瞭“漂變”與“選擇”在塑造今日生物圈中的共同作用。 第四部分：心智的覺醒——人類的崛起與文明的火花 在生命演化的最後階段，故事的主角聚焦於靈長類動物中一個相對年輕的分支——智人。本書追溯瞭從南方古猿到現代人類的漫長遷徙之路，詳細考察瞭直立行走、工具製造、大腦容量的急劇增長如何賦予我們的祖先獨特的生存優勢。 作者深入探討瞭語言和符號思維的起源，這些非物質的工具如何使得知識的積纍和文化的傳遞成為可能。從火的使用到農業的革命，從定居到文字的誕生，本書描繪瞭人類文明的基石是如何一塊塊奠定的。同時，它也審慎地探討瞭人類心智的獨特之處——我們探索宇宙、理解自身局限性的能力，以及這種能力帶來的責任。 第五部分：我們所知的邊界——未來的挑戰與存在的意義 在收尾部分，本書將視角投嚮現代科學的前沿，並反思人類在宇宙中的位置。通過對量子力學、相對論以及復雜係統理論的通俗闡述，作者引導讀者思考我們目前對現實理解的局限性。 我們討論瞭氣候變化的科學基礎、基因編輯技術的倫理睏境，以及人類對外星生命的持續探索。最終，本書迴歸到最初的哲學命題：在一個充滿無限可能性的宇宙中，我們短暫的、脆弱的生命體驗究竟意味著什麼？《宇宙的奇妙旅程》以一種既謙遜又充滿敬畏的姿態，鼓勵讀者擁抱未知，並珍視我們所擁有的這個知識與生命共存的奇跡時刻。 本書特色： 跨學科的整閤敘事： 將看似獨立的科學領域無縫連接，展現科學知識的整體性。 注重過程而非結論： 深入描繪科學發現背後的思想掙紮、實驗的麯摺和理論的推翻與重建。 宏大的時間尺度： 通過生動的比喻，將數十億年的演化壓縮成易於理解的篇章。 哲學思辨的深度： 在描述“是什麼”的同時，不忘探討“為什麼”和“意味著什麼”。 適閤讀者： 所有對自然世界充滿好奇心、渴望建立一套完整世界觀的求知者。無論您是科學領域的專業人士，還是希望通過一本引人入勝的讀物全麵瞭解科學曆史與基礎的普通讀者，本書都將是一次不可多得的精神盛宴。它不僅是知識的普及，更是一次對人類智慧和存在本身的贊頌。

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最讓我感到驚喜的是作者對科學史人物的描摹，那些名字不再是教科書上冰冷的符號，而是被賦予瞭血肉和復雜的人性。他們是如何在偏見中堅持、如何在貧睏中掙紮、又是如何因為一個靈光乍現的念頭而改變瞭人類對世界的認知，這些細節的捕捉，讓整個科學發展史鮮活瞭起來。我仿佛能看到那些科學傢們在昏暗的燈光下與數據搏鬥，在不被理解的壓力下堅持信念的場景。這種對“人”的聚焦，使得那些抽象的科學概念變得可親近、可共情，它們不再是高高在上的真理，而是由一群有血有肉、充滿激情與缺陷的人們一步步摸索齣來的成果，極大地激發瞭我對科學探索精神的嚮往。

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這本書的封麵設計簡直是視覺的盛宴，那種沉靜中蘊含著無限能量的感覺，讓人一拿在手就捨不得放下。油墨的觸感和紙張的細微紋理，都透露齣一種對知識的敬畏與珍視。我尤其欣賞那種字體排版的巧思，它既保持瞭學術的嚴謹性，又不失閱讀的舒適度，即便是長時間沉浸其中，眼睛也不會感到疲憊。裝幀的工藝也極其考究，書脊的摺疊處處理得恰到好處，體現瞭齣版商對“經典”二字的理解和堅持。每一次翻閱，都像是在進行一次精心策劃的儀式，從指尖觸及紙張的那一刻起，就預示著一場深邃的精神之旅即將開啓。這種對實體書形態的極緻追求，在如今這個數字化的時代裏，顯得尤為珍貴和難能可貴，它不僅僅是一本書，更像是一件值得收藏的藝術品，靜靜地待在書架上，本身就是一種無聲的宣言。

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這本書的知識密度極高，但絕非那種令人望而生畏的堆砌，而更像是一種精心調配的“知識雞尾酒”。每一種元素——從物理學、化學到生物學和地質學——都被巧妙地融閤在一起，形成瞭一種流暢、和諧的整體風味。初讀時，我仿佛置身於一個巨大的知識迷宮，每走一步都有新的發現，偶爾會被一些深奧的概念絆倒。但隨著閱讀的深入，我開始看到那些隱藏在不同學科背後的統一邏輯和相互關聯，那些曾經孤立的知識點如同被磁力吸引，緊密地聚閤起來，構成瞭一幅宏偉的“萬物圖景”。這種融會貫通的體驗，遠超齣瞭單純獲取信息的範疇，它重塑瞭我理解世界運作的基本框架，是真正意義上的“開智”之作。

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這本書的敘事節奏把握得如同頂尖交響樂的指揮棒，時而如磅礴的大提琴閤奏，將宇宙洪荒的宏大敘事緩緩鋪陳開來；時而又化為靈動的長笛獨奏，巧妙地切入那些鮮為人知的小科學傢的軼事，充滿瞭人性的光輝與掙紮。我發現自己完全被這種抑揚頓挫的節奏牽引著，在不同的尺度間自如穿梭，從誇剋層麵的微觀世界到星係團的尺度，轉換之間毫無滯澀之感。作者的筆觸輕盈而精準，他懂得如何懸置一個引人入勝的問題，然後層層剝開迷霧，讓讀者在恍然大悟中感受到知識的魅力。這種敘事上的張力，使得即便是麵對那些理論物理或地質年代學等可能枯燥的題材時，也讓人保持著高度的好奇心，生怕錯過任何一個精彩的轉摺點。

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閱讀這本書的過程，與其說是在學習科學知識，不如說是在參與一場跨越時空的哲學思辨。它迫使我不斷地後退一步，重新審視我們習以為常的世界觀和時間觀。那些關於生命起源、地球的漫長演化、以及人類在浩瀚宇宙中位置的探討，都如同高懸的警鍾，時刻提醒著我們存在的偶然性和奇跡性。我時常會在讀到某個驚人的數據或某個科學理論的突破時，停下來，望嚮窗外，感受那種腳下堅實土地的巨大曆史背景。這種“去中心化”的視角，極大地拓寬瞭我對“現實”的定義，讓我對人類文明的成就和局限性有瞭更深一層的理解，不再將當下的狀態視為理所當然的終點。

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送貨比較快，藥效過段時間再評

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書的質量不錯，京東做活動的時候買書還是挺值的

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蠻好的，紙張不錯。

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很好的一次購書，一次還選京東！

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不錯，唯一一本沒被京東物流壓壞的。以後買書盡可能不要選京東。

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最好彆買，懷疑是盜版的

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買給弟弟的，弟弟還在上初中，他很愛科學，希望他能不忘初心，勇敢前行。

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學校要求的必讀書目

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包裝破瞭