The 2400year search for the atom Theresa Doud

What do an ancient Greek philosopher

and a 19th century Quaker

have in common
with Nobel Prize-winning scientists?

Although they are separated
over 2,400 years of history,

each of them contributed
to answering the eternal question:

what is stuff made of?

It was around 440 BCE
that Democritus first proposed

that everything in the world
was made up of tiny particles

surrounded by empty space.

And he even speculated
that they vary in size and shape

depending on the substance they compose.

He called these particles “atomos,”
Greek for indivisible.

His ideas were opposed by
the more popular philosophers of his day.

Aristotle, for instance, disagreed completely,

stating instead that matter
was made of four elements:

earth, wind, water and fire,

and most later scientists followed suit.

Atoms would remain
all but forgotten until 1808,

when a Quaker teacher named John Dalton
sought to challenge Aristotelian theory.

Whereas Democritus’s atomism
had been purely theoretical,

Dalton showed that common substances
always broke down into the same elements

in the same proportions.

He concluded that the various compounds

were combinations of atoms
of different elements,

each of a particular size and mass

that could neither be created
nor destroyed.

Though he received
many honors for his work,

as a Quaker, Dalton lived modestly
until the end of his days.

Atomic theory was now accepted
by the scientific community,

but the next major advancement

would not come
until nearly a century later

with the physicist J.J. Thompson’s
1897 discovery of the electron.

In what we might call
the chocolate chip cookie model of the atom,

he showed atoms as
uniformly packed spheres of positive matter

filled with negatively charged electrons.

Thompson won a Nobel Prize in 1906
for his electron discovery,

but his model of the atom
didn’t stick around long.

This was because he happened
to have some pretty smart students,

including a certain Ernest Rutherford,

who would become known
as the father of the nuclear age.

While studying the effects
of X-rays on gases,

Rutherford decided
to investigate atoms more closely

by shooting small, positively charged
alpha particles at a sheet of gold foil.

Under Thompson’s model,

the atom’s thinly dispersed
positive charge

would not be enough
to deflect the particles in any one place.

The effect would have been
like a bunch of tennis balls

punching through a thin paper screen.

But while most of the particles
did pass through,

some bounced right back,

suggesting that the foil was more
like a thick net with a very large mesh.

Rutherford concluded that atoms
consisted largely of empty space

with just a few electrons,

while most of the mass
was concentrated in the center,

which he termed the nucleus.

The alpha particles
passed through the gaps

but bounced back from the dense,
positively charged nucleus.

But the atomic theory
wasn’t complete just yet.

In 1913, another of Thompson’s students
by the name of Niels Bohr

expanded on Rutherford’s nuclear model.

Drawing on earlier work
by Max Planck and Albert Einstein

he stipulated that electrons
orbit the nucleus

at fixed energies and distances,

able to jump from one level to another,
but not to exist in the space between.

Bohr’s planetary model took center stage,

but soon, it too encountered
some complications.

Experiments had shown that rather than
simply being discrete particles,

electrons simultaneously
behaved like waves,

not being confined
to a particular point in space.

And in formulating
his famous uncertainty principle,

Werner Heisenberg showed
it was impossible to determine

both the exact
position and speed of electrons

as they moved around an atom.

The idea that electrons
cannot be pinpointed

but exist within
a range of possible locations

gave rise to the current
quantum model of the atom,

a fascinating theory
with a whole new set of complexities

whose implications
have yet to be fully grasped.

Even though our understanding
of atoms keeps changing,

the basic fact of atoms remains,

so let’s celebrate
the triumph of atomic theory

with some fireworks.

As electrons circling an atom
shift between energy levels,

they absorb or release energy in the form
of specific wavelengths of light,

resulting in
all the marvelous colors we see.

And we can imagine Democritus
watching from somewhere,

satisfied that over two millennia later,

he turned out
to have been right all along.

古希腊哲学家

和 19 世纪贵格会教徒

与诺贝尔奖得主科学家有什么共同点?

尽管它们
相隔 2,400 多年的历史,

但它们每个都
为回答这个永恒的问题做出了贡献:

物质是由什么制成的?

大约在公元前 440 年
,德谟克利特首次提出

世界上的一切都是

由被空旷的空间包围的微小粒子组成的。

他甚至
推测它们的大小和形状会

根据它们组成的物质而有所不同。

他称这些粒子为“原子”,
希腊语是不可分割的。

他的想法遭到了他
那个时代更受欢迎的哲学家的反对。

例如,亚里士多德完全不同意,

而是说物质
是由四种元素组成的:

土、风、水和火,

后来的大多数科学家也纷纷效仿。

直到 1808 年,

当一位名叫约翰道尔顿的贵格会教师
试图挑战亚里士多德理论时,原子才几乎被遗忘。

德谟克利特的
原子论纯粹是理论上的,而

道尔顿则表明,普通物质
总是以相同的比例分解成相同的元素

他得出的结论是,各种化合物


不同元素的原子的组合,

每种元素都有特定的大小和质量

,既不能创造
也不能破坏。

尽管他的工作获得了
许多荣誉,但

作为一名贵格会教徒,道尔顿一直过着谦虚的生活,
直到生命的尽头。

原子理论现在
被科学界所接受,

直到近一个世纪后

,物理学家 J.J. 才出现下一个重大进展。 汤普森
1897 年发现电子。

在我们可以称之为
原子的巧克力饼干模型中,

他将原子展示为
均匀填充的正物质球体,其中

充满了带负电的电子。

汤普森因发现电子而获得了 1906 年的诺贝尔奖

但他的原子模型
并没有长期存在。

这是因为他
碰巧有一些相当聪明的学生

,其中包括

一位后来被
称为核时代之父的欧内斯特·卢瑟福。


研究 X 射线对气体的影响时,

卢瑟福决定

通过在一张金箔上发射小的带正电的
阿尔法粒子来更仔细地研究原子。

在汤普森的模型下

,原子的稀薄分散的
正电荷

不足以使粒子在任何地方偏转。

效果
就像一堆

网球穿过薄薄的纸屏幕。

但是,虽然大部分粒子
确实通过了,但

有些粒子立即反弹回来,

这表明箔
更像是一张带有非常大网眼的厚网。

卢瑟福得出结论,原子
主要由

只有几个电子的空空间组成,

而大部分
质量集中在中心

,他称之为原子核。

阿尔法粒子
穿过间隙,

但从密集的
带正电的原子核中反弹回来。

但是原子理论
还没有完成。

1913 年,汤普森的另一个
学生尼尔斯·玻尔

扩展了卢瑟福的核模型。

借鉴
马克斯普朗克和阿尔伯特爱因斯坦的早期工作,

他规定电子

以固定的能量和距离围绕原子核运行,

能够从一个水平跃迁到另一个水平,
但不能存在于两者之间的空间中。

玻尔的行星模型占据了中心舞台,

但很快,它也遇到了
一些复杂情况。

实验表明
,电子不仅是离散的粒子,而且

同时
表现得像波一样,

不局限于
空间中的特定点。

在制定
他著名的不确定性原理时,

维尔纳·海森堡表明
,当电子围绕原子移动时,不可能同时

确定电子的确切
位置和速度

电子
无法被精确定位

但存在于
一系列可能位置的想法

产生了当前的
原子量子模型,这

是一个
具有全新复杂性

的迷人理论,其含义
尚未完全掌握。

尽管我们对原子的理解
不断变化,但

原子的基本事实仍然存在,

所以让我们用一些烟花
庆祝原子理论的胜利

当电子绕着原子
在能级之间移动时,

它们会
以特定波长的光吸收或释放能量,

从而产生
我们所看到的所有奇妙的颜色。

我们可以想象德谟克利特
从某个地方观看

,他对两千年后

证明他
一直都是对的感到满意。