Star Discovered In Closest Known Orbit Around Likely Black Hole

Ep. 5 Star Classifications Part 1: Leavitt and Variable Stars - HD and the Void

First in a two-part series about stars and how we classify them. Variables are a very specific kind of star that have a regular variation in brightness, like a heartbeat. They were first categorized and analyzed by Henrietta Swan Leavitt at the tu...

Stars are too distant to really peer at and they have all that radiation and heat and blinding light and such so it’s doubtful that we will ever be able to prod the Sun, but astronomers can certainly classify what stars we’ve been able to observe! This is the first part of a two-part series on star classification systems. This podcast focuses on variable stars, how they were discovered, the awesome women who started developing the basis of a major star classification system, and what variable stars did for our understanding of the universe. 

There is a lot of technical talk and I did my best to make it comprehensible but you can absolutely hit me up with questions if you have them! I’m also on Twitter at @HDandtheVoid if you’d rather ask me there. And go ahead and check out the podcast on iTunes, rate it or review it if you’d like, and subscribe! I’ll always post all the extras here on tumblr but iTunes might be more convenient for downloading and podcast apps and all that good stuff.

Below the cut is some elaboration on the episode itself, including my sources, music credits, a BIG glossary, a quote on women and emotional labor that really hits home for me, and a transcript. I mention a couple of books and quote a couple people in this episode so if you want to see that written down, those sources are there as well. Let me know what you think of this episode, let me know what you think I should research next*, tell me a fun space fact… anything’s helpful! 

*(The June 19th podcast is already set, it’s going to be part 2 on star classifications, but in July I could start talking about things like spectroscopy, planets, dark matter, or I have a book in at the library on longitude.)

Glossary:

arcsecond - an infinitesimal measurement of a degree; in 1 degree there are 3,600 arcseconds.

cosmic distance measurements: light-years - a way to imagine distance scales on an astronomical level; the distance light can travel in one year, or about 6 trillion miles. parsecs - a measurement of distance on an astronomical scale; the distance to a star that shifts by one arcsecond from one side of Earth’s orbit to the other. It’s more common than using light-years when discussing deep space astronomy. One parsec is about 19 trillion miles (30 trillion kilometers), a bit over 3 light-years.

magnitude - the measurement of a star’s brightness as seen from earth. The brighter it is, the lower its magnitude value; the Sun has an apparent magnitude of -27.

Malmquist Bias - the stars that are visible in a cluster are the brightest ones. Astronomers rely on them to compute average luminosity, but the fact that they’re the brightest ones inevitably skews the results.

parallax - the apparent shift of an object when viewed through two different lines of sight.

radial velocity - the speed at which a star is moving away from or towards Earth.

standard candle - a kind of celestial object that has a known luminosity due to some characteristic that the entire class of objects possesses.

stellar photometry - measuring and recording the magnitude of stars.

triangulation - a technique to measure the distance of an object by observing it from two different locations, knowing the distance between both observation locations and measuring the angle at which the distant object moves (its parallax angle).

variable stars: variable stars - stars that change brightness. Reasons for the brightness changes vary, and certain types of variable stars can be used to determine relative distance. They are either intrinsic (when a change in brightness is caused by a star’s own physical changes, like pulsation or eruption) or extrinsic (when the variance has an external cause, such as an eclipse of one star by another or stellar rotation). Cepheid variables - variable stars with a period between 1 and 70 days, with light variations from 0.1 to 2 magnitudes. They’re massive, with a high luminosity and are usually classified between F and G or K. They obey the period-luminosity relationship and played a major part in calculating distances to far-away galaxies as well as helping to determine the age of the Universe. eclipsing binaries - binary systems of stars where the components regularly eclipse one another, causing an apparent decrease in the brightness of the system. irregular variables - variable stars, typically red giants, without a measurable period to their luminosity. Long Period Variables - LPVs have periods ranging from 30 to 1,000 days. They’re red giants or supergiants, typically classified M, R, C, or N. There are subclasses, too: Mira, which have light variations of more than 2.5 magnitudes and are the future evolution of our own star, the Sun; and semiregular, which have some regular periods and some irregular light variation and have light variations less than 2.5 magnitudes. RR Lyrae - variable stars with a period of 0.05 to 1.2 days and a light variation between 0.3 and 2 magnitudes. They’re older and smaller than Cepheids, and are white giant stars typically classified as A. RV Tauri - variable stars that have periods between 30 and 150 days, light variation up to 3 magnitudes, and possible cycle variations that can be hundreds or thousands of days long. They’re yellow supergiants classified between G and K.

cataclysmic variables: dwarf nova - a close binary system of a red dwarf, a white dwarf, and an accretion disk around the white dwarf. They brighten by 2 to 6 magnitudes depending on the stability of the disk, which loses material to the white dwarf. nova - a close binary system of a white dwarf and a secondary star that’s a little cooler than the Sun. The system brightens 7 to 16 magnitudes in 1 to 100 days, and then the star fades slowly to the initial brightness over a period of several years or decades. At maximum brightness, it’s similar to an A or F giant star. Recurrent novae are similar to this category of variable but have several outbursts during their recorded history. R Coronae Borealis - an eruptive variable, a supergiant star that is hydrogen-poor and carbon-rich and spends most of its time at maximum light, fading as much as 9 magnitudes at irregular intervals. Most often classified between F and K or R. supernova - a massive star that explodes with a magnitude increase of 20 or more. Supernovae have led us to realize that the expansion of the Universe is accelerating. symbiotic stars -  close binary systems of a red giant and a hot blue star. They have nova-like outbursts up to 3 magnitudes.

Script/Transcript

Sources:

What stars are made of via NASA

Stars, Cepheid Variable by T. Lloyd Evans via the California Institute of Technology aka CalTech

Variable stars via the Australia Telescope National Facility

American Association of Variable Star Observers website. I used a couple of pages from this one but the whole organization is kinda on the nose.

Stellar magnitude via EarthSky

A star magnitude scale via Harvard

Harvard Observatory’s Astronomical Photographic Plate Collection, which has a history of the collection and the women computers.

Definitions and differences for parsecs and light-years, and a description of parallax and triangulation via EarthSky

Standard candle breakdowns via some magical wonderful person with the best accessible online science book project I have ever encountered. Mad props to whoever is doing this, it’s a noble cause.

Info on Walter Baade via the Online Archives of California

A very math-y breakdown of the Malmquist Bias in the article “Observational Selection Bias Affecting the Determination of the Extragalactic Distance Scale” by P. Teerikorpi, published 1997

Johnson, George. Miss Leavitt’s Stars. Atlas Books: NY, 2005.

Henrietta Swan Leavitt quote: “It is worthy of notice [that] the brighter variables have the longer periods” (38).

“If a theory or observation seemed to suggest that we, the observers, happen to occupy an exalted place in the heavens, then it was probably wrong” (110)

Edwin Hubble quote: “With increasing distance, our knowledge fades, and fades rapidly. Eventually, we reach the dim boundary—the utmost limits of our telescopes. There, we measure shadows, and search among ghostly errors of measurements for landmarks that are scarcely more substantial” (130)

Pickover, Clifford A. “Leavitt’s Luminosity Law.” Archimedes to Hawking: Laws of Science and the Great Minds Behind Them. Oxford UP: NY, 2008. 475.

Soba, Dava. The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars. Viking: New York, 2016.

From Claire Messud’s The Woman Upstairs (I haven’t read the book, I just collect quotes, so this isn’t me endorsing the book; I know nothing about it except this paragraph): “I’m a good girl, I’m a nice girl, I’m a straight-A, strait-laced, good daughter, good career girl, and I never stole anybody’s boyfriend and I never ran out on a girlfriend, and I put up with my parents’ shit and my brother’s shit, and I’m not a girl anyhow, I’m over forty fucking years old, and I’m good at my job and I’m great with kids and I held my mother’s hand when she died, after four years of holding her hand while she was dying and I speak to my father every day on the telephone–every day, mind you, and what kind of weather do you have on your side of the river, because here it’s pretty gray and a bit muggy too? It was supposed to say ‘Great Artist’ on my tombstone, but if I died right now it would say ‘such a good teacher/daughter/friend’ instead; and what I really want to shout, and want in big letters on that grave, too, is FUCK YOU ALL.”

Intro Music: ‘Better Times Will Come’ by No Luck Club off their album Prosperity

Filler Music: 'River Man’ by Nick Drake off his album Five Leaves Left.

Outro Music: ‘Fields of Russia’ by Mutefish off their album On Draught

Ep. 8 Planets - HD and the Void

Eight planets in the solar system or nine? I go into depth with nine because I grew up with Pluto. The first five planets are visible to the naked eye but how did we find Uranus, Neptune, and Pluto? What are we doing to still learn about our close...

Earth is a super special world. It has life on it, and getting conditions just right so that life will survive is an incredibly difficult task. Other planets and other moons in our solar system may look like they could have life on them, but it just didn’t happen.

Life on other planets is for a different episode, though. In this one, I’m talking about what we can see on our close neighbors, the eight (maybe seven?) planets in our solar system. Learn how they were discovered, what naming conventions we use for them and their moons, how to differentiate between them, and what probes we’ve sent out to learn more about them. Also enjoy snippets from the lovely orchestral suite written for each planet by Gustav Holst! It’s the longest episode so far but I promise it’s worth it.

There’s a timeline below the cut in addition to the other resources because hooboy did I mention a lot of people. I may also put together a timeline of probes... But that’s for another podcast. Maybe the next podcast! Let me know what you think I should research by messaging me here, tweeting at me at @HDandtheVoid, or asking me to my face if you know me in real life. And please check out the podcast on iTunes, rate it or review it if you’d like, subscribe, and maybe tell your friends about it if you think they’d like to listen! Also below the cut are my sources, music credits, vocab list, and the transcript. I mention a book, a play, a poem, and a few works of art, and I quote an astronomy book in this episode so if you want to see that written down, those sources are there as well.

(My thoughts for the next episode were spectroscopy, auroras, or probes through the ages. Let me know by the 21st and I’ll have the next podcast up by July 31!)

Glossary:

auroras - a light display that occurs when a magnetosphere is sufficiently disturbed by solar wind that charged particles scatter into the upper atmosphere and lose their energy.

magnetosphere - an invisible barrier that surrounds a celestial objet. It is often generated by the movement of the liquid metal core of the object. Around a planet, it deflects high-energy, charged particles called cosmic rays that can either come from the Sun or, less often, from interstellar space.

prograde - when a planet spins from east to west.

retrograde - when a planet spins from west to east.

sol - a unit of time measuring one Martian day, or 24 Earth-hours and 40 Earth-minutes. The immediately previous Martian day is called yestersol.

transit of Mercury/Venus - when a planet passes in front of the Sun.

Script/Transcript

Timeline of people mentioned

Nicolaus Copernicus, Polish (1473-1543)

Tycho Brahe, Danish (1541-1601)

Galileo Galilei, Italian (1564-1642)

Johannes Kepler, German (1571-1630)

Simon Marius, German (1573-1625)

Pierre Gassendi, French (1592-1655)

Giovanni Cassini (also known as Jean-Dominique Cassini), Italian/French (1625-1712)

Christiaan Huygens, Dutch (1629-1695)

William Herschel, German/English (1738-1822)

Johann Elert Bode, German (1747-1826)

Caroline Herschel, German/English (1750-1848)

Johann Franz Encke, German (1791-1865)

John Herschel, English (1792-1871)

William Lassell, English (1799-1880)

Urbain Le Verrier, French (1811-1877)

Johann Galle, German (1812-1910)

John Couch Adams, English (1819-1892)

Edouard Roche, French (1820-1883)

Heinrich Louis d’Arrest, German (1822-1875)

Asaph Hall III, American (1829-1907)

James Clark Maxwell, Scottish (1831-1879)

Giovanni Schiaparelli, Italian (1835-1910)

Percival Lowell, American (1855-1916)

Eugène Antoniadi (also known as Eugenios Antoniadis), Greek (1870-1944)

Gerard Kuiper, Dutch/American (1905-1973)

Clyde Tombaugh (1906-1997)

Sources:

Who discovered each planet via Cornell University

The mathematical discovery of Neptune and Pluto via University of St. Andrews, where my mom’s boyfriend’s son graduated last year! Mad props, Henry!

Holst’s The Planets via the Utah Symphony

More on Holst’s suite, including music files

Chronology of solar system discovery

MESSENGER information via John Hopkins University Applied Physics Laboratory

Auroras via NASA’s Themis mission

Magnetospheres via NASA, which has a tumblr! You should follow it! Good stuff.

Curiosity rover via NASA

‘Canali on Mars’ debacle via NASA

Mariner 9 via NASA

Origin of ‘yestersol’ and Martian day-length via A Way With Words

Richard Bram: “Superlatives are inadequate; words fail. Look. Think. Be in awe.”

Images of Mars through the years via The Telegraph

Mars-One mission to colonize Mars

Names of all the planet’s moons and their significance in mythology, last updated in 2013 and questionably reliable but from what I know of mythology—and I do know more than most—it’s not too far off.

Table of moons of various planets

Jupiter via NASA

Jupiter moon name facts via NASA

The Galilean Moons of Jupiter via University of Colorado at Boulder

Saturn’s moons via Phys.org

Cassini mission website

Saturn overview via NASA

Saturn’s moon Titan via NASA

Ethane via PubChem

Methane via EPA

Neptune’s moons via Space.com

What is Pluto via NASA

Pluto Overview via NASA

“Dwarf planets may provide the best evidence about the origins of our solar system.”

New Horizons mission via NASA

Pluto and our designations for planets are mentioned very briefly in this Oatmeal comic. I liked it.

Sobel, Dava. The Planets. Viking: NY, 2005.

“But tides raised by the Sun in the planet’s molten middle gradually damped Mercury’s rotation down to its present slow gait” (34).

“Light and heat always hit Mercury dead on, while the north and south poles, which receive no direct sunlight, remain relatively frigid at all times” (35).

“Venusian clouds comprise large and small droplets of real vitriol—sulfuric acid along with caustic compounds of chlorine and fluorine. They precipitate a constant acid rain, called virga, that evaporates in Venus’ hot, arid air before it has a chance to strike the ground” (61).

“…Neptune, where the voices of a female choir, sequestered in a room offstage, are made to fade out at the finale (with no sacrifice in pitch) by the slow, silent closing of a door” (165).

Holst: “Saturn brings not only physical decay but also a vision of fulfillment” (165).

“They occupy a nearby region of perpetual fragmentation known as the Roche zone, named for the nineteenth-century French astronomer Edouard Roche, who formulated the safe distances for planetary satellites” (172).

“It's near twin, Neptune, reveals a more complex beauty in subtle stripes and spots of royal to navy blue, azure, turquoise, and aquamarine” (200).

“This outlying population offered Pluto a new identity—if not the last planet, then the first citizen of a distant teeming shore” (214).

Van Gogh, Vincent. Starry Night (June 1889). 

—. Road with Cypress and Star (May 1890). 

—. White House at Night (June 1890). 

Shakespeare, William. A Midsummer Night’s Dream (1605).

Pope, Alexander. “The Rape of the Lock” (1712). (It’s a mock-epic satiric poem about stealing a lock of hair, not physical rape)

Duane, Diane. Wizards at War. Harcourt Trade Publishers: San Diego CA, 2005.

Intro Music: ‘Better Times Will Come’ by No Luck Club off their album Prosperity

Filler Music: The Planets (1918) by Gustav Holst, performed by the London Symphony Orchestra in 2003.

Outro Music: ‘Fields of Russia’ by Mutefish off their album On Draught

Ep. 28 Tidal Forces - HD and the Void

Tidal forces are not only the cause of ocean tides, but affect how satellites orbit objects in space, and they can even tear some objects apart under their extreme stresses. Learn about types of tides on Earth and in our solar system.

This episode’s been a long time coming because the topic’s come up before. I originally conceived of this podcast as a way for me to learn about space things I’d always taken for granted, and truly, there is nothing closer to home that I’ve just agreed to believe than the statement that the tides are affected by the Moon. What? How? Why? All these questions and some I didn’t even realize I had will be answered in this episode on tidal forces!

Below the cut are my standard glossary, transcript, sources, and music credits. Send me any topic suggestions via Tumblr message (you don’t need an account for it!). You can also tweet at me on Twitter at @HDandtheVoid, or you can ask me to my face if you know me. Subscribe on iTunes to get the new episodes of my maybe now monthly-updated podcast (we’ll see how the weeks unfold), and please please please rate and review it. Go ahead and tell friends if you think they’d like to hear it, too!

(My thoughts on the next episode are Stephen Hawking and his theories, or famous comets. The next episode will go up in September—ideally, September 10th!)

Glossary

barycenter - the common center of mass between two objects that allows them to orbit.

Roche limit - the distance in which a celestial body will disintegrate because of a second celestial body's tidal forces exceeding the first body's gravitational self-attraction, or the force that’s holding it together. Within the Roche limit, orbiting material disperses and forms rings, like how Saturn’s rings are within the Roche zone; outside the limit, material tends to coalesce.

spaghettification - when extreme tidal forces pull an object apart in space.

tidal force - an apparent force (sometimes also called the differential force) that stretches a body towards another, more gravitationally-strong body’s center of mass. This can cause such diverse phenomena as tides, tidal locking, breaking celestial bodies apart to form ring systems within a Roche limit, and in extreme cases, spaghettification. It arises because the gravitational force exerted on one body by another is not constant across its parts: the nearest side is attracted more strongly than the farthest side.

Types of ocean tides:

diurnal tide - a daily tidal cycle with only one high and low tide each lunar day, and a period of a little over 24 hours.

meteorological tide - a tidal change due to weather patterns. Wind, or unusually high or low barometric pressure causes variations between the actual sea level and its predicted height.

mixed tide - a daily tidal cycle with two high and low tides that differ in their peaks. This difference in height between successive high or low tides is called the diurnal inequality. They have a period of 12 hours and 25 minutes.

neap tide - a type of bi-monthly tidal cycle that occurs when the Sun, Earth, and Moon are positioned at a 90-degree angle, so the tidal forces of the Sun are acting against the tidal forces of the Moon. During a neap tide, the difference between high tide and low tide is the least extreme.

semidiurnal tide - a daily tidal cycle with two nearly equal high tides and low tides every lunar day. They have a period of 12 hours and 25 minutes.

spring tide - a type of bi-monthly tidal cycle that occurs when the Sun, Earth, and Moon line up so that the gravitational forces of Sun and Moon are working together to form a large tidal bulge. During a spring tide, the difference between high tide and low tide is at its maximum.

tidal locking - when long-term interaction between two co-orbiting astronomical bodies causes at least one of the bodies to rotate in such a way that one face of the body is always pointed at the body it’s orbiting. This is also called gravitational locking or captured rotation. An example is that the same side of the Moon always faces the Earth, and its synchronous rotation means that it takes just as long to rotate around its own axis as it does to revolve around the Earth.

Script/Transcript

Sources

Tidal Cycles in Tides Explained via beltoforian.de

“a tide is a distortion in the shape of one body induced by the gravitational pull of another nearby object.”

Meteorological effects on tides via the New Zealand Government website

Tides and Water Levels via the National Oceanic and Atmospheric Administration (NOAA)

Tides by R. Nave, my dude, my guy, my friend and yours, of Georgia State University

The Tidal Force by Neil deGrasse Tyson via Hayden Planetarium (Nov 1995)

“A mild increase in distance between two objects can make a large difference in the strength of the tidal force. For example, if the Moon were just twice its current distance from us, then its tidal force on Earth would decrease by a factor of eight. At its current average distance of 240,000 miles from Earth, the Moon manages to create sizable atmospheric, oceanic, and crustal tides by attracting the part of Earth nearest the Moon more strongly than the part of Earth that is farthest. (The Sun is so far away that in spite of its generally strong gravity, its tidal force on Earth amounts to less than half that of the Moon.) The oceans respond most visibly in being stretched toward the direction of the Moon.” 

“When Earth's rotation slows down until it exactly matches the orbital period of the Moon, then Earth will no longer be rotating within its oceanic tidal bulge and the Earth-Moon system will have achieved a double tidal lock. In what sounds like an undiscovered wrestling hold, double tidal locks are energetically favorable (like a ball coming to rest at the bottom of a hill), and are thus common in the universe.”

Forget “Earth-Like”—We’ll First Find Aliens on Eyeball Planets via Nautilus (Feb 2015)

High Tide on Io! via NASA (Mar 2012)

Tidal forces and spaghettification via NASA handout

Spaghettification via Cosmic Funnies

Single atoms feel tidal force via Physics World (May 2017)

Robbins, Tom. Still Life with Woodpecker. Bantam Books: New York, 1980.

“Being four times larger than the moon, the earth appeared to dominate. Caught in the earth’s gravitational web, the moon moved around the earth and could never get away. Yet, as any half-awake materialist well knows, that which you hold holds you.”

Sobel, Dava. The Planets. Viking: NY, 2005.

Intro Music: ‘Better Times Will Come’ by No Luck Club off their album Prosperity

Background Music: ‘Sad Business’ by Patients aka Ben Cooper, who primarily releases music as Radical Face but also has at least three other bands or band names he’s working with/has released music as.

Filler Music: ‘It’s Getting Boring by the Sea’ by Blood Red Shoes off their album Box of Secrets

Outro Music: ‘Fields of Russia’ by Mutefish off their album On Draught

Ongoing Space Science Seeks to Keep Astronauts Healthy

ISS - Expedition 50 Mission patch. March 10, 2017 NASA is preparing for longer human journeys deeper into space and is exploring how to keep astronauts healthy and productive. The Expedition 50 crew members today studied space nutrition, measured their bodies and checked their eyes to learn how to adapt to living in space. The space residents also unloaded a cargo ship, worked on the Tranquility module and practiced an emergency simulation. The ongoing Energy experiment that ESA astronaut Thomas Pesquet collected urine samples for today seeks to define the energy requirements necessary to keep an astronaut successful during a space mission. Pesquet also joined NASA astronaut Peggy Whitson for body measurements to learn how microgravity affects body shape and impacts crew suit sizing. Commander Shane Kimbrough checked his eyes today with Whitson’s help and support from experts on the ground.

Image above: Astronaut Shane Kimbrough and Thomas Pesquet were pictured inside the cupola just after the SpaceX Dragon was captured Feb. 23, 2017. Image Credit: NASA. Kimbrough worked throughout the day before his eye checks and configured the Tranquility module for upcoming electronics and communications work. Cosmonaut Oleg Novitskiy continued unloading gear from the newly-arrived Progress 66 cargo ship. At the end of the day, Novitskiy joined Whitson and Pesquet for an emergency simulation with inputs from control centers in Houston and Moscow. Related links: Energy experiment: https://www.nasa.gov/mission_pages/station/research/experiments/397.html Body measurements: https://www.nasa.gov/mission_pages/station/research/experiments/1070.html Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html Image (mentioned), Text, Credits: NASA/Mark Garcia. Best regards, Orbiter.ch Full article

Ep. 1 MUL.APIN - HD and the Void

Welcome to the first episode of HD and the Void, space edition! Start at the beginning of the universe with the Big Bang, then zoom to the beginning of records of humanity's astronomical observations with the Mesopotamian star chart MUL.APIN. Bonu...

The first episode is here! I have never done this before and right now, I’m planning to put up a podcast every two weeks.

Below the cut is some elaboration on the episode itself, including my sources, music credits, a glossary, and a transcript (not an exact record of this episode, but it’s the script I was working with and it’s both conversational and also a little less rambling than what I actually said). I’m on Twitter now, too: @HDandtheVoid. I don’t know what I’ll put there yet except maybe fun little facts and, of course, notifications on when an episode goes up.

Let me know what you think of this episode, let me know what you think I should research next*, tell me a fun space fact… anything’s helpful at this point!

*(Move fast if you feel strongly about what I research next, though, cuz I have to get it done by April 24th—I don’t mention it in the podcast but this is me telling you now so I am held accountable; April 24th is the next podcast.)

Glossary:

cosmic microwave background radiation—the electromagnetic radiation left over from the time of recombination in Big Bang cosmology.

cosmology—the study of the properties of our universe as a whole.

heliacal rising—when a star or constellation rises at the same time or just before the sun.

parapegma—a list of star rising times.

retrograde—the apparent motion of a planet in a direction opposite to that of other bodies within its system, as observed from a particular vantage point.

sidereal year—the time required for the earth to complete an orbit of the sun relative to the stars.

star catalog—an astronomical catalog that lists stars.

star chart/map—A star chart or star map is a map of the night sky. Astronomers divide these into grids to use them more easily. They are used to identify and locate astronomical objects such as stars, constellations, and galaxies.

tropical year—the interval at which seasons repeat and the basis for the calendar year.

Wilkinson Microwave Anisotropy Probe—a spacecraft operating from 2001 to 2010 which measured temperature differences in the cosmic microwave background radiation leftover from the Big Bang. (I said ‘anistropy’ in the podcast, whoops)

Script/Transcript (It’s not exactly what I said, but it’s what I was going off of. It’s conversational and it’s less rambly than what I actually said)

Sources:

Cosmic microwave background radiation info

More Big Bang info

Timeline of the Big Bang

Babylonian constellation/zodiac list

Babylonian star catalog

Retrograde motion

Evans, James. The History and Practice of Ancient Astronomy. Oxford UP: New York, 1998.

...and class notes from a class on Ancient Astronomy I took with Prof. James Evans.

My argument for using Wikipedia is that it is shockingly accurate when it comes to ancient material. I’m going to try to stick to academic and government sources though.

Intro Music: ‘Better Times Will Come’ by No Luck Club off their album Prosperity

Outro Music: ‘Fields of Russia’ by Mutefish off their album On Draught

I talked about spaghettification but someone did one better and made a dang cute comic about it!

Starry Greetings!

This week’s comic: Spaghettification 

https://www.youtube.com/watch?v=OGn_w-3pjMc

http://science.howstuffworks.com/science-vs-myth/what-if/what-if-fell-into-black-hole2.htm

What is so special about the solar eclipse to you??

Huh, that’s a very good question and I probably answer it differently each time I get asked it. I love the fact that in totality you can see the solar atmosphere and get a chance to see the magnetic field structure of the Sun. This is something that you can’t normally do. I also love the idea that we’re going to be able to test a bunch of ionospheric models with the help of citizen scientist! This again is a very unique opportunity! But probably the thing that seems so special about this particular eclipse is seeing how excited everyone is about it! Most days I sit in my office working on my science (which I think is the best science and most interesting thing in the world- but I’m probably biased about that) and not too many other people in the world are all that excited about it. But with the eclipse, I get to share how cool this science is, and it’s amazing to see everyone get involved! 

Soyuz MS-10 experiences launch anomaly; crew aborts to safe landing.

One of Russia’s most reliable launchers experienced a rare, in-flight anomaly earlier this morning, forcing the two-man crew of Soyuz MS-10 to abort the mission.

Following a normal liftoff at 4:40am EST (2:40pm local time), a malfunction in the Soyuz FG rocket two minutes into the flight forced Expedition 57 crewmembers Alexey Ovchinin and Nick Hague to abort a manual abort profile. The anomaly occurred immediately following the separation of the rocket’s four strap-on boosters and jettisoning of the Launch Escape System. However, the protective fairing covering the spacecraft during flight through the thick atmosphere was still on, and solid rocket motors attached to the fairing pulled the crew capsule away from the failing booster. Following a ballistic trajectory through the upper atmosphere, the Soyuz’s Descent module separated from the Orbital Module and payload fairing and descended to a safe landing 20 kilometers east of Zezkezhan, Kazakhstan, 34 minutes after launch. Roscosmos reported that the crewmembers experienced around seven times the force of gravity, or 7G’s, during their abort. 

Recovery forces reached the landing site immediately following touchdown. Both astronauts were reported to be in good health following their ordeal, and returned to their families at the Baikonur launch site around six hours after liftoff.

Recovery forces at the Soyuz MS-10 emergency landing site. Source: Ruptly.

Soyuz MS-10 crewmembers Alexey Ovchinin and Nick Hague embrace their families following their return to the Baikonur Cosmodrome after today’s launch mishap. Credit: NASA/Bill Ingalls. This marks the first crewed launch mishap of the International Space Station program, the first crewed launch mishap since the Challenger disaster in 1986, and the first crewed Soyuz launch malfunction since Soyuz T-10 in 1983.

That incident saw the two-man crew of Vladimir Titov and Gennady Strekalov abort away from their exploding rocket shortly before its scheduled liftoff time.  While no cause of the mishap is currently known, Russian authorities have begun an investigation of the incident and have temporarily grounded all future Soyuz flights.  The current three-member crew of Expedition 57 is slated to return to Earth December 13, followed by the launch of Expedition 58 December 20. Following today’s anomaly, it is unclear whether Expedition 57 will remain on orbit longer, or when the next crew will launch to the station. Expedition 57 is able to remain on orbit until early January, when their Soyuz reaches its certified orbital lifetime.

Expedition 57 commander Alexander Gerst captured this image of the Soyuz MS-10 launch from the International Space Station. The anomalous nature of the launch is evidenced by multiple points of light along the ascent path. Source: NASA. Watch NASA TV coverage of the Soyuz MS-10 launch below.

P/c: NASA.

Just a reminder that the first NASA astronauts were supposed to be women because generally they are smaller, lighter (less weight in the cockpit means less fuel required) and eat less than men and so would be easier to accommodate in space. 

After spending a month attached to the ISS, the Dragon spacecraft succesfully lands in the pacific and is shipped back to land.

via reddit