Meet SA-500D, The First Saturn V Rocket. Wernher Von Braun Designed Her As The Dynamic Test

Heads up, this is tomorrow night! I hope it's clear where I am to see it but considering I'm in the Pacific Northwest, I don't have super high hopes. Get a look if you can, though! Rare to see a blue moon that's actually red :)

A Total Lunar Eclipse is Coming: 10 Things to Know

If you were captivated by August’s total solar eclipse, there’s another sky show to look forward to on Jan. 31: a total lunar eclipse!

Below are 10 things to know about this astronomical event, including where to see it, why it turns the Moon into a deep red color and more…

1. First things first. What’s the difference between solar and lunar eclipses? We’ve got the quick and easy explanation in this video:

2. Location, location, location. What you see will depend on where you are. The total lunar eclipse will favor the western U.S., Alaska, Hawaii, and British Columbia on Jan. 31. Australia and the Pacific Ocean are also well placed to see a major portion of the eclipse, if not all of it.

3. Color play. So, why does the Moon turn red during a lunar eclipse? Here’s your answer:

4. Scientists, stand by. What science can be done during a lunar eclipse? Find out HERE. 

5. Show and tell. What would Earth look like from the Moon during a lunar eclipse? See for yourself with this artist’s concept HERE. 

6. Ask me anything. Mark your calendars to learn more about the Moon during our our Reddit AMA happening Monday, Jan. 29, from 3-4 pm EST/12-1 pm PST.

7. Social cues. Make sure to follow @NASAMoon and @LRO_NASA for all of the latest Moon news leading up to the eclipse and beyond.

8. Watch year-round. Can’t get enough of observing the Moon? Make a DIY Moon Phases Calendar and Calculator that will keep all of the dates and times for the year’s moon phases right at your fingertips HERE.

Then, jot down notes and record your own illustrations of the Moon with a Moon observation journal, available to download and print from moon.nasa.gov.

9. Lesson learned. For educators, pique your students’ curiosities about the lunar eclipse with this Teachable Moment HERE.

10. Coming attraction. There will be one more lunar eclipse this year on July 27, 2018. But you might need your passport—it will only be visible from central Africa and central Asia. The next lunar eclipse that can be seen all over the U.S. will be on Jan. 21, 2019. It won’t be a blue moon, but it will be a supermoon.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.  

Here’s a great example of the kinds of experiments astronauts perform on the International Space Station, just like I talked about in Episode 19! I absolutely want to high-five whoever called is ISS-CREAM.

From Frozen Antarctica to the Cold Vacuum of Space

A new experiment that will collect tiny charged particles known as galactic cosmic rays will soon be added to the International Space Station. The Cosmic Ray Energetics And Mass for the International Space Station payload, nicknamed ISS-CREAM, will soon be installed in its new home on the Station’s Japanese Experiment Module Exposed Facility. ISS-CREAM will help scientists understand more about galactic cosmic rays and the processes that produce them.

Wait, what are cosmic rays?

Cosmic rays are pieces of atoms that move through space at nearly the speed of light. Galactic cosmic rays come from beyond our solar system. 

They provide us with direct samples of matter from distant places in our galaxy.

Why do these things go so fast?

Galactic cosmic rays have been sped up by extreme processes. When massive stars die, they explode as supernovas. The explosion’s blast wave expands into space along with a cloud of debris. 

Particles caught up in this blast wave can bounce around in it and slowly pick up speed. Eventually they move so fast they can escape the blast wave and race away as a cosmic ray.

Where can we catch cosmic rays?

Cosmic rays are constantly zipping through space at these super-fast speeds, running into whatever is in their path – including Earth.  

But Earth’s atmosphere is a great shield, protecting us from 99.9 percent of the radiation coming from space, including most cosmic rays.  This is good news for life on Earth, but bad news for scientists studying cosmic rays.  

So… how do you deal with that?

Because Earth has such an effective shield against cosmic rays, the best place for scientists to study them is above our atmosphere – in space.  Since the 1920s, scientists have tried to get their instruments as close to space as possible. One of the simplest ways to do this is to send these instruments up on balloons the size of football stadiums. These balloons are so large because they have to be able to both lift their own weight and that of their cargo, which can be heavier than a car. Scientific balloons fly to 120,000 feet or more above the ground – that’s at least three times higher than you might fly in a commercial airplane!  

Credit: Isaac Mognet (Pennsylvania State University)

Earlier versions of ISS-CREAM’s instruments were launched on these giant balloons from McMurdo Station in Antarctica seven times, starting in 2004, for a total of 191 days near the top of the atmosphere.  Each of these flights helped the team test their hardware and work towards sending a cutting-edge cosmic ray detector into space!  

How is going to space different than flying balloons?

Balloon flights allowed the team to collect a lot of cosmic rays, but even at 120,000 feet, a lot of the particles are still blocked. Scientists at the University of Maryland, College Park, who operate ISS-CREAM, expect to get about 10 times as much data from their new home on the International Space Station. 

That’s because it will be both above the atmosphere and fly far longer than is possible with a balloon. As you might imagine, there are large differences between flying something on a balloon and launching it into space. The science instruments and other systems had to be changed so ISS-CREAM could safely launch on a rocket and work in space.

What will ISS-CREAM do?

While on the space station, ISS-CREAM will collect millions of cosmic rays – electrons, protons and atomic nuclei representing the elements found in the solar system. These results will help us understand why cosmic rays reach the wicked-fast speeds they do and, most important, what limits those speeds.

ISS-CREAM launches to the International Space Station aboard the latest SpaceX Dragon spacecraft, targeted to launch August 14. Want to learn more about ISS-CREAM and some of our scientific balloons? Check out our recent feature, NASA’s Scientific Balloon Program Reaches New Heights.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Ep. 25 Southern Stars - HD and the Void

I live in the Northern Hemisphere of Earth, which means I see some constellations and stars that people in the Southern Hemisphere don't see. The opposite is true as well, and it's more interesting for me to talk about the constellations I don't g...

I’m a Northern Hemisphere dweller, so I thought it would be fun to cover Southern Hemisphere stars and constellations in this episode! I also coulsnt’ resist talking about Aurora Australis and Steve, the hot new atmospheric phenomenon all the young people are talking about.

Below the cut, I have the glossary, transcript, sources, and music credits. I take topic suggestions from Tumblr messages, or you can tweet at me on Twitter at @HDandtheVoid, or you can ask me to my face if you know me. Please subscribe on iTunes, rate my podcast and maybe review it, and tell friends if you think they’d like to hear it!

(My thoughts on the next episode are Chuck Yeager, Stephen Hawking and his theories, the opposition of Mars, or famous comets. The next episode will go up May 14th or 21st!)

Glossary

Bayer designation - a way to classify stars based on their relative brightness within a constellation. A specific star is identified by a Greek letter, followed by the genitive form of the constellation's Latin name.

circumpolar - appearing to orbit one of the Earth’s poles. For stars and constellations, this means they are above the horizon at all times in certain latitudes.

irregular galaxy - an asymmetrical galaxy shape, where the galaxy lacks a central supermassive black hole.

Script/Transcript

Sources

Orion from the Southern Hemisphere via EarthSky (Mar 2017)

How to Spot Sky Landmarks: Big Dipper and Southern Cross via Space.com (Apr 2012)

Locate Cassiopeia the Queen via EarthSky (February 2018)

Small Magellanic Cloud orbits Milky Way via EarthSky (Oct 2017)

Nubecula via LatDict

Early star catalogues of the southern sky via Astronomy and Astrophysics (2011)

Catalog of Southern Stars via the University of Oklahoma

Edmond Halley via Royal Museums Greenwich

Finding south using the Southern Cross via Museum of Applied Arts and Sciences (Jan 2013)

List of 88 official constellations via the Astronomical Society of Southern Africa

Alpha Centauri system, closest to sun via EarthSky (May 2017)

Hadar is a southern pointer star via EarthSky (April 2017)

Aurora Australis forecast service

Video of aurora australis via Global News Canada (April 2018)

Aurora Steve via Global News Canada (March 2018)

Bagnall, Philip M. “Crux.” In The Star Atlas Companion: What You Need to Know About the Constellations. Springer Science+Business Media: New York, 2012 (183-7). Located in Google Books Preview [accessed May 1, 2018].

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

Filler Music: ‘Mace Spray’ by The Jezabels off their EP Dark Storm.

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

Ep. 30 Coriolis Effect - HD and the Void

The Coriolis force is a force in physics that has profound impact on us here on Earth. Listen to hear how this apparent force has influence over the weather, tides, and even some creatures. I refuse to talk about the formulas surrounding it but I ...

We’re back in 2019 with an episode that would have been more appropriate to release during hurricane season: a discussion of the Coriolis force! This force was observed centuries ago but takes its name from the scientist who first considered it in terms of theory and physics. It has an impact on a vast range of natural phenomena, from weather patterns to ocean waves to the flights of flies and moths.

Below the cut are the glossary, transcript, a timeline of the people I mention, sources, and music credits. Send me any topic suggestions via Tumblr message (you don’t need an account to do this, just submit as anonymous). You can also tweet at me on Twitter at @HDandtheVoid, or you can ask me to my face if you know me in real life. Subscribe on iTunes to get the new episodes of my so-far-monthly-updated podcast, 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, Hedy Lamarr, or famous comets. The next episode will go up in late February.)

Glossary

Coriolis force - a force in a rotating system that acts perpendicular to the direction of motion and to the axis of rotation. On Earth, this tends to deflect moving objects to the right in the Northern Hemisphere and to the left in the Southern Hemisphere.

Ekman transport - the net motion of fluid that results from the balance between Coriolis and turbulent drag forces.

Eötvös effect - the change in perceived gravitational force that results from eastbound or westbound movement on Earth’s surface.

Kelvin waves - an ocean wave that is trapped at the Earth’s equator and along vertical boundaries like coastlines. They move towards the equator when they have a western boundary; towards the poles when they have an eastern boundary; and make a whirlpool when they have a closed boundary, moving counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere.

Lagrange points -  five points where three bodies can orbit each other, yet stay in the same position relative to each other in a stable configuration. L1-L3 are in line with each other, while L4 and L5 are at the points of equilateral triangles in the configuration.

prograde - when a planet spins from east to west.

Rossby number - used to determine the relative importance of the centrifugal and Coriolis forces in maps of weather patterns. A small Rossby number indicates that a weather system is strongly affected by Coriolis forces, while a large Rossby number signifies that a system is affected by inertial and centrifugal forces.

Transcript

Timeline

Giovanni Battista Riccioli, Italian (1598-1671)

Francesco Maria Grimaldi, Italian (1618-63)

Joseph-Louis Lagrange, French (1736-1813)

Gaspard-Gustave de Coriolis, French (1792-1843)

Sir William Thompson, AKA Lord Kelvin, Scots-Irish (1824-1907)

Baron Loránd Eötvös de Vásárosnamény, Hungarian (1848-1919)

Ottokar Tumlirz, Austrian (1856-1928)

Fridtjof Nansen, Norwegian (1861-1930)

Vagn Walfrid Ekman, Swedish (1874-1954)

Carl-Gustaf Arvid Rossby, Swedish-born American (1898-1957)

Sources

Coriolis Effect via the University of Oregon

Coriolis Force via Wikipedia

Coriolis effect, two centuries before Coriolis via Physics Today (Aug 2011)

Gaspard-Gustave de Coriolis via Wikipedia

Coriolis effect via National Geographic

Hurricane, cyclone, typhoon, tornado – what’s the difference? via African Reporter (Sep 2017)

Wang, B. Kelvin Waves. University of Hawaii: Honolulu, 2002.

Ocean in Motion: Ekman Transport Background via NASA

Ekman transport via Wikipedia

What is a Geodesist? via Environmental Science

“The Second Coming” by W. B. Yeats via Poetry Foundation

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

Filler Music: ‘Ambergris’ by Tipper off their EP Fathoms

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

Geocentric map of the Solar System.

Ep.17 Edmond Halley - HD and the Void

Edmond Halley was heavily involved in the establishment of modern astronomy, whether through his direct observational work or through the support he offered others in his field. Hear a quick overview of the man who's popped up so much throughout t...

I’m back! July was nuts! June was also nuts! I’ve missed this podcast, though, and have been thinking about it the entire time because I will never stop loving space. I was working my way through a very meaty book on Edmond Halley and I am here to report on my findings, and also compile some of the things I’ve already said about this cool guy and his cool contributions to science.

Below the cut are my standard glossary, transcript, timeline of people mentioned, sources, and music credits. I take topic suggestions from Tumblr messages, you can 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 increasingly erratically updated podcast, 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 August—hopefully August 20th!)

Glossary

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

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

Script/Transcript

Timeline

Julius Caesar, Roman (100-45 BCE)

Augustus Caesar, Roman (63-14 BCE) 

Nicolaus Copernicus, Polish (1473-1543)

Pope Gregory XIII, Italian (1502-1585)

Tycho Brahe, Danish (1546-1601)

Johannes Kepler, German (1571-1630)

Johannes Hevelius, Polish (1611-1687)

Giovanni Cassini (in French, Jean-Dominique Cassini), Italian/French (1625-1712)

Queen Christina, Swedish (1626-1689)

Isaac Newton, English (1643-1727)

John Flamsteed, English (1646-1719)

Elisabeth Hevelius, Polish (1647-1693)

Edmond Halley, English (1656-1742)

John Harrison, English (1693-1776)

Sources

Morse, Stephen P. “The Julian Calendar and why we need to know about it.” The Association of Professional Genealogists Quarterly (March 2014). Accessed July 15, 2018.

Julian Date Converter via the Astronomical Applications Department of the U.S. Naval Observatory.

Hughes, David W. “Edmond Halley, Scientist.” British Astronomical Association (1985). Accessed July 27, 2018.

Cook, Alan. Edmond Halley: Charting the Heavens and the Seas. Clarendon Press: Oxford, 1998.

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

Cassini Just Sent Back Closest Ever Images of Saturn, And They're Incredible

NASA's Cassini probe is plunging to its death. The nuclear-powered spacecraft has orbited Saturn for 13 years, and sent back hundreds of thousands of images. The photos include close-ups of the gaseous giant, its famous rings, and its enigmatic moons - including Titan, which has its own atmosphere, and icy Enceladus, which has a subsurface ocean that could conceivably harbour microbial life.

YO THAT SHIT BALLER AS FUCK HOLY SHIT

Physicists Have Figured Out Where The Sun's Plasma Jets Come From

Things are heating up.

After over a century of observations and several theories, scientists may have finally nailed the origin of the high-speed plasma blasting through the Sun’s atmosphere several times a day. Using a state-of-the-art computer simulation, researchers have developed a detailed model of these plasma jets, called spicules.

The new findings answer some of the bigger questions in solar physics, including how these plasma jets form and why the Sun’s outer atmosphere is far hotter than the surface.

“This is the first model that has been able to reproduce all the features observed in spicules,” Juan Martinez-Sykora, lead author and astrophysicist at the Bay Area Environmental Research Institute in California, told ScienceAlert.

Continue Reading.

why is there star

gas cloud get squished (gravitational collapse) then sometimes smaller elements can squish together to make bigger elements (nuclear fusion) and this continues as long as the smolest elements (hydrogen and helium) are in the core