The first asteroid ever discovered Carrie Nugent

On the night of January 1, 1801,

Giuseppe Piazzi,
a priest in Palermo, Italy,

was mapping the stars in the sky.

Over three nights, he’d look at and draw
the same set of stars,

carefully measuring
their relative positions.

That night, he measured the stars.

The next night, he measured them again.

To his surprise, one had moved.

The third night, the peculiar star
had moved again.

This meant it couldn’t be a star at all.

It was something new, the first asteroid
ever discovered,

which Piazzi eventually named Ceres.

Asteroids are bits of rock and metal
that orbit the Sun.

At over 900 kilometers across,
Ceres is a very large asteroid.

But through a telescope, like Piazzi’s,

Ceres looked like a pinpoint of light
similar to a star.

In fact, the word asteroid
means star-like.

You can tell the difference between stars

and asteroids by
the way they move across the sky.

Of course, Piazzi knew
none of that at the time,

just that he had discovered something new.

To learn about Ceres,

Piazzi needed to track
its motion across the sky

and then calculate
its orbit around the Sun.

So each clear night, Piazzi
trained his telescope to the heavens.

Night after night,
he made careful measurements

until finally, he couldn’t.

The Sun got in the way.

When Piazzi first spotted Ceres,
it was here, and the Earth was here.

As he tracked it each night,
the Earth and Ceres moved like this

until Ceres was here.

And that meant that Ceres was only
in the sky when it was daytime on Earth.

During the day, bright sunlight made
this small asteroid impossible to see.

Astronomers needed to calculate
Ceres’s orbit.

This would let them predict where
it was going to be

in the vast night sky on any given night.

But the calculations were grueling
and the results imprecise.

Many astronomers searched for Ceres,

but not knowing exactly where to look,
no one could find it.

Luckily, a hardworking mathematician
named Carl Friedrich Gauss

heard about the lost asteroid.

He thought it was an exciting puzzle
and went to work.

When he realized he didn’t have
the mathematical methods he needed,

he invented new ones
that we still use today.

He derived a new orbit and new predictions
of where to look for Ceres.

Hungarian astronomer
Baron Franz Xaver von Zach

searched for Ceres
with Gauss’s predictions.

After weeks of frustrating clouds,

von Zach finally had clear skies
on December 31, 1801.

He looked through his telescope
and finally saw Ceres.

We haven’t lost track of it since.

Today, we’ve discovered hundreds
of thousands of asteroids.

Many, including Ceres, orbit the Sun
between Mars and Jupiter,

while near-Earth asteroids orbit
the Sun relatively close to Earth.

When we recorded this narration,

astronomers had discovered
16,407 near-Earth asteroids,

but since we find
new asteroids all the time,

that number will have grown
by hundreds or thousands

by the time you watch this.

Today, asteroid hunters
use modern telescopes,

including one in space.

Computers analyze the images,

and humans check the output

before reporting the asteroid observations
to an archiving center.

Each discovered asteroid has its unique
orbit measured.

An orbit lets astronomers predict
where asteroids are going to be

at any given time.

Most asteroid trajectories can be
predicted for about 80 years

though we can calculate where the best
studied asteroids will be every day

between now and
800 years into the future.

We must keep searching for asteroids

in case there’s one out there
on a collision course with Earth.

Astronomers don’t only
search for asteroids, though.

They also study them
to learn how they formed,

what they’re made of,

and what they can tell us
about our solar system.

Today, we can do something that Piazzi
could only dream of:

send spacecraft to study
asteroids up close.

One spacecraft called Dawn
journeyed billions of kilometers

over four years to the main asteroid belt.

There, it visited Ceres
and another asteroid, Vesta.

Dawn’s stunning images transformed
Piazzi’s dot of light

into a spectacular landscape
of craters,

landslides,

and mountains.

1801 年 1 月 1 日晚上

,意大利巴勒莫的牧师朱塞佩·皮亚齐

正在绘制天空中的星星。

三个晚上,他会观察并
画出同一组星星,

仔细测量
它们的相对位置。

那天晚上,他测量了星星。

第二天晚上,他再次测量了它们。

令他惊讶的是,其中一个已经动了。

第三个晚上,那颗奇特的星星
又动了。

这意味着它根本不可能是明星。

这是新事物,是有史以来发现的第一颗小行星

,皮亚齐最终将其命名为谷神星。

小行星是
围绕太阳运行的岩石和金属碎片。

谷神星直径超过 900 公里,
是一颗非常大的小行星。

但是通过像 Piazzi 的望远镜,

谷神星看起来像一个类似于恒星的精确光点

事实上,小行星这个词的
意思是类星。

您可以

通过
它们在天空中移动的方式来区分恒星和小行星。

当然,当时皮亚齐对此一无所知

,他只是发现了一些新的东西。

为了了解谷神星,

皮亚齐需要跟踪
它在天空中的运动

,然后计算
它围绕太阳的轨道。

因此,每一个晴朗的夜晚,皮亚齐都会
将他的望远镜对准天空。

一夜又一夜,
他仔细测量,

直到最后,他不能。

太阳挡住了路。

当皮亚齐第一次发现谷神星时,
它就在这里,地球也在这里。

当他每晚追踪它时
,地球和谷神星就这样移动,

直到谷神星来到这里。

这意味着谷神星只
在地球上的白天出现在天空中。

白天,明亮的阳光使
这颗小行星无法被看到。

天文学家需要计算
谷神星的轨道。

这可以让他们预测

在任何给定的夜晚它将在广阔的夜空中的位置。

但是计算很费力
,结果也不精确。

许多天文学家寻找谷神星,

但不知道具体去哪里,
没有人能找到它。

幸运的是,一位名叫卡尔弗里德里希高斯的勤奋数学家

听说了这颗丢失的小行星。

他认为这是一个令人兴奋的谜题
并开始工作。

当他意识到自己没有
所需的数学方法时,

他发明
了我们今天仍在使用的新方法。

他推导出了一个新的轨道和
关于在哪里寻找谷神星的新预测。

匈牙利天文学家
弗朗茨·泽维尔·冯·扎克男爵

根据高斯的预测寻找谷神星。

经过数周令人沮丧的乌云,

冯·扎克终于在
1801 年 12 月 31 日拥有晴朗的天空。

他通过望远镜观察
,终于看到了谷神星。

从那以后,我们就再也没有忘记它。

今天,我们已经发现了
数十万颗小行星。

包括谷神星在内的许多小行星
在火星和木星之间绕太阳运行,

而近地小行星则
在相对靠近地球的地方绕太阳运行。

当我们记录这段叙述时,

天文学家已经发现了
16,407 颗近地小行星,

但由于我们一直在发现
新的小行星,所以当你看到这个数字时,

这个数字将
增加数百或数千

今天,小行星猎人
使用现代望远镜,

包括太空望远镜。

计算机分析图像

,人类

在将小行星观测结果报告
给存档中心之前检查输出。

每一颗发现的小行星都有其独特的
轨道测量。

轨道可以让天文学家
预测小行星

在任何给定时间的位置。

大多数小行星的轨迹可以
预测大约 80 年,

尽管我们可以计算出

从现在到
800 年后每天研究得最好的小行星的位置。

我们必须继续寻找小行星

,以防
有一颗与地球相撞。

不过,天文学家不仅在
寻找小行星。

他们还研究它们
以了解它们是如何形成的,

它们是由什么制成的,

以及它们可以告诉我们
关于太阳系的什么信息。

今天,我们可以做
Piazzi 梦寐以求的事情:

发射宇宙飞船
近距离研究小行星。

一艘名为黎明号的宇宙飞船在四年内飞行了
数十亿公里

,到达了主要的小行星带。

在那里,它访问了谷神星
和另一颗小行星灶神星。

黎明的惊人图像将
皮亚齐的光点

变成了
由火山口、

山体滑坡

和山脉组成的壮观景观。