Curl Up, Read A New Series Of Books, And Be Edified! Out Now, Part 1, Vesha Celeste, And Part 2, Eliza
Curl up, read a new series of books, and be edified! Out now, Part 1, Vesha Celeste, and Part 2, Eliza Williams, have been paired together, and are available for those interested in the types and directions of science and the speculation that lead to well-being and quality of life. Please feel free to follow, message, share ideas, and be a part of a positive future where, if we choose, we can prepare properly to navigate the stars. This is just the beginning of this series and prequel, “Pathway to the Stars,” to an even more giant series, “Further than Before!” Please enjoy. https://www.amazon.com/author/matthewopdyke #sciencefiction #scifi #sciencefictionfantasy #scififantasy #politicalscifi #physiology #neurology #physics #Apolitical #strongfemalelead #biotechnology #neuroscience #theoreticalphysics #problemresolution #productivepursuits #spaceopera #cerebraldrama #sophisticateddialogue #solarsystem #spacemining #physiologicaloptimization, #neurologicaloptimization #transhumanism #universalethics #wellbeing #genetherapy #CRISPR #politicalsciencefiction #matthewopdyke https://www.instagram.com/p/BpUMW6ZgB1I/?utm_source=ig_tumblr_share&igshid=wy078mgrbgmm
More Posts from Matthewjopdyke and Others
Pathway to the Stars: Part 1, Vesha Celeste
Pathway to the Stars: Part 1, Vesha Celeste
Soon to be released, is the first in a latched-on (or related) series, Pathway to the Stars: Part 1, Vesha Celeste. This will be a slightly more descriptive portion that goes into more detail of the first character introduced, Vesha Celeste. Please pre-order, read, review, comment, and enjoy! Thank you!
Vesha Celeste journeys with Yesha Alevtina and her dream-angel, Sky, following a long life of…
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Constellations: Andromeda
Andromeda is most prominent during autumn evenings in the Northern Hemisphere, along with several other constellations named for characters in the Perseus myth.
Its brightest star, Alpha Andromedae, is a binary star that has also been counted as a part of Pegasus, while Gamma Andromedae is a colorful binary and a popular target for amateur astronomers. Only marginally dimmer than Alpha, Beta Andromedae is a red giant, its color visible to the naked eye. The constellation’s most obvious deep-sky object is the naked-eye Andromeda Galaxy (M31, also called the Great Galaxy of Andromeda), the closest spiral galaxy to the Milky Way and one of the brightest Messier objects.
In this image of the Andromeda Galaxy, Messier 32 is to the left of the center.
Several fainter galaxies, including M31’s companions M110 and M32, as well as the more distant NGC 891, lie within Andromeda. The Blue Snowball Nebula, a planetary nebula, is visible in a telescope as a blue circular object.
NGC 891, as taken with amateur equipment
Along with the Andromeda Galaxy and its companions, the constellation also features NGC 891 (Caldwell 23), a smaller galaxy just east of Almach. It is a barred spiral galaxy seen edge-on, with a dark dust lane visible down the middle.
In addition to the star clusters NGC 752 and NGC 7686, there is also the planetary nebula NGC 7662.
Each November, the Andromedids meteor shower appears to radiate from Andromeda. The shower peaks in mid-to-late November every year, but has a low peak rate of fewer than two meteors per hour. Astronomers have often associated the Andromedids with Biela’s Comet, which was destroyed in the 19th century, but that connection is disputed. source
A Cosmic Legacy: From Earth to the Stars
“Our beautiful mother world ached for a reprieve from the injustices of many, courtesy of cultures and governance systems that forgot how to love, how to be kind, how to include others, and how to think beyond the scope of greed and power, but within the visions of shared joy and well-being.”
Yesha Alevtina delivers a speech to her audience, following Eliza's address to members of the Pathway organization, during the formation of a new worldwide political party founded on innovation and evolution in the interest of shared well-being. Eliza Williams and a host of friendly heroes go on to tackle some of the most significant dilemmas of the day to bring humanity out and into the stars. Eliza works to help humanity bear a legacy of kindness, of mind-to-mind communication, of love, and of healing instead of harming. If we are to overcome the great expansion and the death of all life, we must overcome the smaller challenges to progress and focus on even greater ones.
Buy this fantastic story and make this grand literary opus the favorite item in your library next to your reading corner, on your nightstand, or in your living room, as you settle in and read while the days go by. Enjoy the story of several heroes who do as much as they can to heal the Earth, provide healing to those suffering most, and help humanity get out and into the Cosmos!
LCCN: 2019911854 ISBN: 978-1-7333131-2-4 https://smile.amazon.com/dp/1733313125
A Cosmic Legacy: From Earth to the Stars #SpaceOpera #ScienceFiction #Fantasy #ACosmicLegacy #Author #SpaceExploration #Longevity #Biotech #Neurotech #Nanotech #Physics and more...
Solar System: Things to Know the August Eclipse
We’re counting down until the August 21 total solar eclipse that will be visible across most of North America. Here are some things you can do to prepare.
1. Find A Spot
The eclipse should be visible to some extent across the continental U.S. Here’s map of its path.
Our eclipse page can help you find the best viewing locations by longitude and latitude: eclipse.gsfc.nasa.gov/SEgoogle/SEgoogle2001/SE2017Aug21Tgoogle.html
2. Citizen Science
Want to know more about citizen science projects? Find a list of citizen science projects for the eclipse: https://eclipse.aas.org/resources/citizen-science
3. Never look directly at the sun! Even during the early phases of the eclipse!
Get your eclipse viewing safety glasses beforehand: eclipse2017.nasa.gov/safety
4. Get Our Interactive Eclipse Module App
In this interactive, 3D simulation of the total eclipse on August 21, 2017, you can see a view of the eclipse from anywhere on the planet:
http://eyes.jpl.nasa.gov/eyes-on-eclipse.html
5. Got questions?
Join the conversation on social media. Tag your posts: #Eclipse2017.
Twitter: @NASASolarSystem, @NASA, @NASASunEarth Facebook: NASA Solar System
Discover the full list of 10 things to know about our solar system this week HERE.
Follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
To all women, who dedicate hours on end toward helping others with little thought of reward in return -- you are a blessing in the lives of all you meet. For that, I wish you a Happy Mother's day! https://www.instagram.com/p/CAArmv5A7C8/?igshid=1v92oi99tgo35
Meet Fermi: Our Eyes on the Gamma-Ray Sky
Black holes, cosmic rays, neutron stars and even new kinds of physics — for 10 years, data from our Fermi Gamma-ray Space Telescope have helped unravel some of the biggest mysteries of the cosmos. And Fermi is far from finished!
On June 11, 2008, at Cape Canaveral in Florida, the countdown started for Fermi, which was called the Gamma-ray Large Area Space Telescope (GLAST) at the time.
The telescope was renamed after launch to honor Enrico Fermi, an Italian-American pioneer in high-energy physics who also helped develop the first nuclear reactor.
Fermi has had many other things named after him, like Fermi’s Paradox, the Fermi National Accelerator Laboratory, the Enrico Fermi Nuclear Generating Station, the Enrico Fermi Institute, and the synthetic element fermium.
Photo courtesy of Argonne National Laboratory
The Fermi telescope measures some of the highest energy bursts of light in the universe; watching the sky to help scientists answer all sorts of questions about some of the most powerful objects in the universe.
Its main instrument is the Large Area Telescope (LAT), which can view 20% of the sky at a time and makes a new image of the whole gamma-ray sky every three hours. Fermi’s other instrument is the Gamma-ray Burst Monitor. It sees even more of the sky at lower energies and is designed to detect brief flashes of gamma-rays from the cosmos and Earth.
This sky map below is from 2013 and shows all of the high energy gamma rays observed by the LAT during Fermi’s first five years in space. The bright glowing band along the map’s center is our own Milky Way galaxy!
So what are gamma rays?
Well, they’re a form of light. But light with so much energy and with such short wavelengths that we can’t see them with the naked eye. Gamma rays require a ton of energy to produce — from things like subatomic particles (such as protons) smashing into each other.
Here on Earth, you can get them in nuclear reactors and lightning strikes. Here’s a glimpse of the Seattle skyline if you could pop on a pair of gamma-ray goggles. That purple streak? That’s still the Milky Way, which is consistently the brightest source of gamma rays in our sky.
In space, you find that kind of energy in places like black holes and neutron stars. The raindrop-looking animation below shows a big flare of gamma rays that Fermi spotted coming from something called a blazar, which is a kind of quasar, which is different from a pulsar… actually, let’s back this up a little bit.
One of the sources of gamma rays that Fermi spots are pulsars. Pulsars are a kind of neutron star, which is a kind of star that used to be a lot bigger, but collapsed into something that’s smaller and a lot denser. Pulsars send out beams of gamma rays. But the thing about pulsars is that they rotate.
So Fermi only sees a beam of gamma rays from a pulsar when it’s pointed towards Earth. Kind of like how you only periodically see the beam from a lighthouse. These flashes of light are very regular. You could almost set your watch by them!
Quasars are supermassive black holes surrounded by disks of gas. As the gas falls into the black hole, it releases massive amount of energy, including — you guessed it — gamma rays. Blazars are quasars that send out beams of gamma rays and other forms of light — right in our direction.
When Fermi sees them, it’s basically looking straight down this tunnel of light, almost all the way back to the black hole. This means we can learn about the kinds of conditions in that environment when the rays were emitted. Fermi has found about 5,500 individual sources of gamma rays, and the bulk of them have been blazars, which is pretty nifty.
But gamma rays also have many other sources. We’ve seen them coming from supernovas where stars die and from star factories where stars are born. They’re created in lightning storms here on Earth, and our own Sun can toss them out in solar flares.
Gamma rays were in the news last year because of something Fermi spotted at almost the same time as the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo on August 17, 2017. Fermi, LIGO, Virgo, and numerous other observatories spotted the merger of two neutron stars. It was the first time that gravitational waves and light were confirmed to come from the same source.
Fermi has been looking at the sky for almost 10 years now, and it’s helped scientists advance our understanding of the universe in many ways. And the longer it looks, the more we’ll learn. Discover more about how we’ll be celebrating Fermi’s achievements all year.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Happy International Women’s Day!
Today we celebrate International Women’s Day, a day in which we honor and recognize the contributions of women…both on Earth and in space.
Since the beginning, women have been essential to the progression and success of America’s space program.
Throughout history, women have had to overcome struggles in the workplace. The victories for gender rights were not achieved easily or quickly, and our work is not done.
Today, we strive to make sure that our legacy of inclusion and excellence lives on.
We have a long-standing cultural commitment to excellence that is largely driven by data, including data about our people. And our data shows progress is driven by questioning our assumptions and cultural prejudices – by embracing and nurturing all talent we have available, regardless of gender, race or other protected status, to build a workforce as diverse as our mission. This is how we, as a nation, will take the next giant leap in exploration.
As a world leader in science, aeronautics, space exploration and technology, we have a diverse mission that demands talent from every corner of America, and every walk of life.
So, join us today, and every day, as we continue our legacy of inclusion and excellence.
Happy International Women’s Day!
Learn more about the inspiring woman at NASA here: https://women.nasa.gov/
Enjoy the #sciencefiction #fantasy #spaceopera #ebook #audiobook #novel series #furtherthanbefore by #Author #matthewjopdyke
With intellect, experience, perspective, kindness, and graciousness we will have the ability to gain more wisdom leading to longevity and clarity of mind. For Eliza and her crew of friends, it is a race against time to prepare humanity to meet new civilizations, preserve life, share our legacies, and go further than before! No matter the challenge, there will always be an opportunity for greater pursuits!
My #mom went to be with my #dad yesterday morning. I will miss her dearly. #togetherforever they gave myself and siblings a home of #love and #kindness and they #taught us to be #loving and #kind I'll miss you both 💖 https://www.instagram.com/p/BvUjmvOAaac/?utm_source=ig_tumblr_share&igshid=1xk08dpggqtaz
Interesting project. :)
How To Prove Einstein’s Relativity For Less Than $100
“But the fact that you can see cosmic ray muons at all is enough to prove that relativity is real. Think about where these muons are created: high in the upper atmosphere, about 30-to-100 kilometers above Earth’s surface. Think about how long a muon lives: about 2.2 microseconds on average. And think about the speed limit of the Universe: the speed of light, or about 300,000 kilometers per second. If you have something moving at the speed of light that only lives 2.2 microseconds, it should make it only 0.66 kilometers before decaying away. With that mean lifetime, less than 1-in-10^50 muons should reach the surface. But in reality, almost all of them make it down.”
Relativity, or the idea that space and time are not absolute, was one of the most revolutionary and counterintuitive scientific theories to come out of the 20th century. It was also one of the most disputed, with hundreds of scientists refusing to accept it. Yet with less than $100 and a single day’s worth of labor, there’s a way you can prove it to yourself: by building a cloud chamber. An old fishtank, some 100% ethyl or isopropyl alcohol, a metal base with dry ice beneath it and only a few other steps (see the full article for instructions) will allow you to construct a detector capable of seeing unstable cosmic particles. Yet these particles – and you’ll see about 1-per-second – would never reach Earth’s surface if it weren’t for relativity!
Come learn how you can validate Einstein’s first great revolution all for yourself, and silence the doubts in your mind. Nature really is this weird!
