Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920

Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920
Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920
Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920
Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920
Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920
Astronomical Photographs, Harvard College Observatory, Cambridge, 1890-1920

Astronomical photographs, Harvard College Observatory, Cambridge, 1890-1920

More Posts from Ad-astra-affecte-spe and Others

IC 4628: The Prawn Nebula ©

IC 4628: The Prawn Nebula ©


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Lunar Halo
Lunar Halo

Lunar halo

@picabuzz


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“Drifting” By | André Brandt

“Drifting” by | André Brandt

Perseverance: Drifting Clouds Just Before Sunrise On Mars (March 18, 2023)

Perseverance: Drifting clouds just before sunrise on Mars (March 18, 2023)

2 years ago
Inneston, South Australia, Australia | Blntpencil

Inneston, South Australia, Australia | blntpencil


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The Dancer In Dorado

The dancer in Dorado

800 megapixel

Clearest photo of a galaxy you will ever see!

Cosmic Alphabet Soup: Classifying Stars

Cosmic Alphabet Soup: Classifying Stars

If you’ve spent much time stargazing, you may have noticed that while most stars look white, some are reddish or bluish. Their colors are more than just pretty – they tell us how hot the stars are. Studying their light in greater detail can tell us even more about what they’re like, including whether they have planets. Two women, Williamina Fleming and Annie Jump Cannon, created the system for classifying stars that we use today, and we’re building on their work to map out the universe.

Cosmic Alphabet Soup: Classifying Stars

By splitting starlight into spectra – detailed color patterns that often feature lots of dark lines – using a prism, astronomers can figure out a star’s temperature, how long it will burn, how massive it is, and even how big its habitable zone is. Our Sun’s spectrum looks like this:

Cosmic Alphabet Soup: Classifying Stars

Astronomers use spectra to categorize stars. Starting at the hottest and most massive, the star classes are O, B, A, F, G (like our Sun), K, M. Sounds like cosmic alphabet soup! But the letters aren’t just random – they largely stem from the work of two famous female astronomers.

Cosmic Alphabet Soup: Classifying Stars

Williamina Fleming, who worked as one of the famous “human computers” at the Harvard College Observatory starting in 1879, came up with a way to classify stars into 17 different types (categorized alphabetically A-Q) based on how strong the dark lines in their spectra were. She eventually classified more than 10,000 stars and discovered hundreds of cosmic objects!

Cosmic Alphabet Soup: Classifying Stars

That was back before they knew what caused the dark lines in spectra. Soon astronomers discovered that they’re linked to a star’s temperature. Using this newfound knowledge, Annie Jump Cannon – one of Fleming’s protégés – rearranged and simplified stellar classification to include just seven categories (O, B, A, F, G, K, M), ordered from highest to lowest temperature. She also classified more than 350,000 stars!

Cosmic Alphabet Soup: Classifying Stars

Type O stars are both the hottest and most massive in the new classification system. These giants can be a thousand times bigger than the Sun! Their lifespans are also around 1,000 times shorter than our Sun’s. They burn through their fuel so fast that they only live for around 10 million years. That’s part of the reason they only make up a tiny fraction of all the stars in the galaxy – they don’t stick around for very long.

Cosmic Alphabet Soup: Classifying Stars

As we move down the list from O to M, stars become progressively smaller, cooler, redder, and more common. Their habitable zones also shrink because the stars aren’t putting out as much energy. The plus side is that the tiniest stars can live for a really long time – around 100 billion years – because they burn through their fuel so slowly.

Cosmic Alphabet Soup: Classifying Stars

Astronomers can also learn about exoplanets – worlds that orbit other stars – by studying starlight. When a planet crosses in front of its host star, different kinds of molecules in the planet’s atmosphere absorb certain wavelengths of light.

By spreading the star’s light into a spectrum, astronomers can see which wavelengths have been absorbed to determine the exoplanet atmosphere’s chemical makeup. Our James Webb Space Telescope will use this method to try to find and study atmospheres around Earth-sized exoplanets – something that has never been done before.

Cosmic Alphabet Soup: Classifying Stars

Our upcoming Nancy Grace Roman Space Telescope will study the spectra from entire galaxies to build a 3D map of the cosmos. As light travels through our expanding universe, it stretches and its spectral lines shift toward longer, redder wavelengths. The longer light travels before reaching us, the redder it becomes. Roman will be able to see so far back that we could glimpse some of the first stars and galaxies that ever formed.

Learn more about how Roman will study the cosmos in our other posts:

Roman’s Family Portrait of Millions of Galaxies

New Rose-Colored Glasses for Roman

How Gravity Warps Light

Make sure to follow us on Tumblr for your regular dose of space!

11 months ago
Apollo 11 Launch
Apollo 11 Launch
Apollo 11 Launch
Apollo 11 Launch
Apollo 11 Launch

Apollo 11 Launch

this morning NASA abandoned their mars rover Opportunity (aka Oppy) because it (she) got hit by a storm on Mars and it knocked her camera and wheels out and her last words to the team were “my battery is low and it is getting cold”. I know she’s a machine but I’m devastated. Oppy is the one who discovered water on Mars. RIP oppy ily space baby


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ad-astra-affecte-spe - reach for the stars with hope
reach for the stars with hope

★•Astronomy, Physics, and Aerospace•★ Original and Reblogged Content curated by a NASA Solar System Ambassador

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