SPACE FACTS: DAY 237/365π°οΈπ§ͺπ
There are at least 5500 galaxies in the area covered by a grain of rice held at arm's length, as revealed by the Hubble eXtreme Deep Field, which stared at a patch of sky for a total of 22.5 days over 10 years to see galaxies as faint as magnitude 31!
Image: NASA/ESA
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SPACE FACTS: DAY 237/365π°οΈπ§ͺπ
There are at least 5500 galaxies in the area covered by a grain of rice held at arm's length, as revealed by the Hubble eXtreme Deep Field, which stared at a patch of sky for a total of 22.5 days over 10 years to see galaxies as faint as magnitude 31!
Image: NASA/ESA
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gorgeous!
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RΓΈmer delay still is used to account for observational light delays due to the Earth's position in its orbit!
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SPACE FACTS: DAY 236/365π°οΈπ§ͺπ
You can see the effect of the finite speed of light from the orbits of Jupiterβs moons! In fact this was how the very first measurement of the speed of light was ever taken, by the astronomer Ole RΓΈmer, from the delay of Io's eclipses by Jupiter.
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Me: I should finish this script in another 30 minutes and have plenty of time to record!
Me 4 hours later: *crying and drawing out these stupid angles yet again*
the sky is confuuuuuuuuuuuusing
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SPACE FACTS: DAY 235/365π§ͺππ°οΈ
Back when the entire universe was a dense sea of plasma, dark matter halos created sound waves in the plasma called Baryonic Acoustic Oscillations. We can see their echoes in both the Cosmic Microwave Background and the present-day clustering of galaxies in the universe!
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SPACE FACTS: DAY 235/365π§ͺππ°οΈ
Back when the entire universe was a dense sea of plasma, dark matter halos created sound waves in the plasma called Baryonic Acoustic Oscillations. We can see their echoes in both the Cosmic Microwave Background and the present-day clustering of galaxies in the universe!
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SPACE FACTS: DAY 234/365π§ͺπ°οΈπ
The sun doesn't just have cool dark spotsβit also has hot bright spots called faculae, which vary on the same cycle as spots. The effect of faculae is a bit more than that of sunspots, making the sun a smidge brighter at sunspot maximum vs sunspot minimum.
Image: NASA
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SPACE FACTS: DAY 234/365π§ͺπ°οΈπ
The sun doesn't just have cool dark spotsβit also has hot bright spots called faculae, which vary on the same cycle as spots. The effect of faculae is a bit more than that of sunspots, making the sun a smidge brighter at sunspot maximum vs sunspot minimum.
Image: NASA
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Had fun attempting to capture my eclipse experience last week! Impossible to do it justice, of course, and a missing tripod piece led to some very questionable videography, but fun nonetheless! π
youtu.be/zKNA25LMEQw
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SPACE FACTS: DAY 233/365ππ°οΈπ§ͺ
Quasars are named from the term "quasi-stellar radio sources". Quasi-stellar means that they appear as single points in the sky, like stars, unlike galaxies. They are some of the brightest objects in the universe, powered by accretion disks of supermassive black holes!
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SPACE FACTS: DAY 233/365ππ°οΈπ§ͺ
Quasars are named from the term "quasi-stellar radio sources". Quasi-stellar means that they appear as single points in the sky, like stars, unlike galaxies. They are some of the brightest objects in the universe, powered by accretion disks of supermassive black holes!
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SPACE FACTS: DAY 232/365π§ͺππ°οΈ
When objects orbit further away from their sun, their orbits take a lot longer. The orbital period increases with the 3/2 power of the orbital distance. E.g., Earth orbits at 1 AU in 1 year, Neptune orbits at ~30 AU in 165 years. (This is Kepler's Third Law!)
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SPACE FACTS: DAY 232/365π§ͺππ°οΈ
When objects orbit further away from their sun, their orbits take a lot longer. The orbital period increases with the 3/2 power of the orbital distance. E.g., Earth orbits at 1 AU in 1 year, Neptune orbits at ~30 AU in 165 years. (This is Kepler's Third Law!)
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Same for us in Dripping Springs! Hell of a timing for the clouds to break and I was so glad
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SPACE FACTS: DAY 231/365ππ§ͺπ°οΈ
Bright lines radiating away from sources in space pictures are called diffraction spikes, caused by the optics of the telescopes (commonly from struts or edges). The patterns can be quite recognizable, e.g., the 8-pointed spikes in Webb images.
Image: NASA/ESA/CSA
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SPACE FACTS: DAY 231/365ππ§ͺπ°οΈ
Bright lines radiating away from sources in space pictures are called diffraction spikes, caused by the optics of the telescopes (commonly from struts or edges). The patterns can be quite recognizable, e.g., the 8-pointed spikes in Webb images.
Image: NASA/ESA/CSA
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It's complicated! There's actually a lot of diversity in pre-collapse stars, and not all of them go through WR phase. Some are entirely stripped of their envelopes by winds or companions but not all!
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SPACE FACTS: DAY 230/365ππ°οΈπ§ͺ
Fusion can happen outside of the core of evolved stars. A very massive star at the end of its life can be fusing silicon in its core surrounded by shells of oxygen-burning, neon-burning, carbon-burning, helium-burning shell, and hydrogen-burning!
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SPACE FACTS: DAY 230/365ππ°οΈπ§ͺ
Fusion can happen outside of the core of evolved stars. A very massive star at the end of its life can be fusing silicon in its core surrounded by shells of oxygen-burning, neon-burning, carbon-burning, helium-burning shell, and hydrogen-burning!
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SPACE FACTS: DAY 229/365ππ°οΈπ§ͺ
Sometimes, a point on the sky will shine brilliantly in radio waves for a tiny fraction of a second. These Fast Radio Bursts were first discovered in 2007 and are thought to be emitted by rapidly rotating compact objects (exact cause TBD).
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SPACE FACTS: DAY 229/365ππ°οΈπ§ͺ
Sometimes, a point on the sky will shine brilliantly in radio waves for a tiny fraction of a second. These Fast Radio Bursts were first discovered in 2007 and are thought to be emitted by rapidly rotating compact objects (exact cause TBD).
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I may have girlbossed a bit too close to the sun as it turns out working full time and running what basically amounts to a part time science communication business does not leave one very much time to relax π«
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SPACE FACTS: DAY 228/365π°οΈπ§ͺπ
Uranus spins on its side! Most of the planets spin almost vertically compared to their orbits, like Earth's 23.5Β° axial tilt or only 3Β° for Jupiter. But Uranus's axial tilt is 98Β°! It likely got knocked into this orientation by a huge collision in the early solar system.
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SPACE FACTS: DAY 228/365π°οΈπ§ͺπ
Uranus spins on its side! Most of the planets spin almost vertically compared to their orbits, like Earth's 23.5Β° axial tilt or only 3Β° for Jupiter. But Uranus's axial tilt is 98Β°! It likely got knocked into this orientation by a huge collision in the early solar system.
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SPACE FACTS: DAY 227/365ππ°οΈπ§ͺ
Sometimes super just isn't enough to describe the power of a collapsing starβso we call them hypernovae! Thought to be from the collapse of a very massive, rapidly rotating star, a hypernova ejects material with about ten times the kinetic energy of a regular supernova.
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SPACE FACTS: DAY 227/365ππ°οΈπ§ͺ
Sometimes super just isn't enough to describe the power of a collapsing starβso we call them hypernovae! Thought to be from the collapse of a very massive, rapidly rotating star, a hypernova ejects material with about ten times the kinetic energy of a regular supernova.
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SPACE FACTS: DAY 226/365π§ͺππ°οΈ
Nowadays, the IAU (not the discoverer) has final say on the naming of a new celestial body, based on input including from the discoverers but also by historical trends and themes, e.g., satellites of Jupiter are named for lovers or descendants of Jupiter/Zeus.
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SPACE FACTS: DAY 226/365π§ͺππ°οΈ
Nowadays, the IAU (not the discoverer) has final say on the naming of a new celestial body, based on input including from the discoverers but also by historical trends and themes, e.g., satellites of Jupiter are named for lovers or descendants of Jupiter/Zeus.
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Over on my channel we're talking about the record-setting exoplanets as a bonus for the Exoplanets 101 series! youtu.be/C5diSsLiPCU?... π§ͺππ°οΈ
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SPACE FACTS: DAY 225/365π°οΈπ§ͺπ
Our sun isn't the only star that has flares. In fact, quite the opposite! The stars that have the most frequent flares are young and low-mass stars, like M dwarfs, while older and more massive stars flare less often.
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You only need a few observations! 3 is the minimum needed to use Gauss's method of orbit determination π
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SPACE FACTS: DAY 225/365π°οΈπ§ͺπ
Our sun isn't the only star that has flares. In fact, quite the opposite! The stars that have the most frequent flares are young and low-mass stars, like M dwarfs, while older and more massive stars flare less often.
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SPACE FACTS: DAY 224/365π§ͺπ°οΈπ
While asteroids are classified by their composition, comets are classified by their orbits: short-period comets, orbits <200 years; long-period comets, can be orbits lasting millions of years; or unbound comets, which pass through the solar system and do not return.
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SPACE FACTS: DAY 224/365π§ͺπ°οΈπ
While asteroids are classified by their composition, comets are classified by their orbits: short-period comets, orbits <200 years; long-period comets, can be orbits lasting millions of years; or unbound comets, which pass through the solar system and do not return.
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SPACE FACTS: DAY 223/365π°οΈππ§ͺ
Fusion in (very massive) stars doesn't end after all the carbon is used up. Next, neon is the fusion fuel, then oxygen, then the final fusion stage is silicon burning! Each stage is faster and shorter than the last, with silicon burning only happening for about a day.
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SPACE FACTS: DAY 223/365π°οΈππ§ͺ
Fusion in (very massive) stars doesn't end after all the carbon is used up. Next, neon is the fusion fuel, then oxygen, then the final fusion stage is silicon burning! Each stage is faster and shorter than the last, with silicon burning only happening for about a day.
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It's been a wild time over on my YT channel this month! Making me feel even worse about how long it's taking to make more long videos π
BUT there is a new one coming this Sunday!! (Normally I post Mondays, but I ain't posting a real science-related video on April 1 π
)
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I've seen it described as being more like soot than dust, really.
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Different composition and formation than household dustβa lot less dead skin cells in space!
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Well for some dust in the solar system we have measured it directly! But in general of course we don't have direct access to interstellar dust, so we have to rely on how the dust interacts with light at different wavelengths, between absorption, scattering, and emission.
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SPACE FACTS: DAY 222/365ππ°οΈπ§ͺ
There's a lot of dust in space, but it's not like dust on a bookshelf. In general the grains are much smaller than the grains of household dust. Astronomical dust is typically a micron in size or less, while household dust can be as large as 100 microns!
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SPACE FACTS: DAY 222/365ππ°οΈπ§ͺ
There's a lot of dust in space, but it's not like dust on a bookshelf. In general the grains are much smaller than the grains of household dust. Astronomical dust is typically a micron in size or less, while household dust can be as large as 100 microns!
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exoplanets πͺ
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Using longer wavelengths, like infrared and radio, helps alleviate but does not fully solve the challenge of exploring the Zone of Avoidance.
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SPACE FACTS: DAY 221/365π°οΈπ§ͺπ
The "Zone of Avoidance" is a swath covering about 20% of the sky that appears devoid of other galaxies. But it's not because they're not there; it's because our view of them is blocked by the dust, gas, and stars of our own galaxy!
Image: 2MASS
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Dynamical friction!
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*blows off dust*
is this thing still on?? π I've been shamelessly neglecting my bsky!
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I've been coding in Python for 7 years and I don't think I've ever written a class π
They scare me
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