Pathway To The Stars: Part 1, Vesha Celeste

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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6 years ago
Please Enjoy My New Sci- Fi Fantasy Novel As Our Heroes Prepare For A Giant Space Adventure In This Two

Please enjoy my new sci- fi fantasy novel as our heroes prepare for a giant space adventure in this two book series. Currently available on Amazon! Further than Before: Pathway to the Stars ( 2 book series) amazon.com/author/matthewopdyke #scififantasy #spaceopera #sciencefiction #mustread #scifinovels #fantasynovels #sciencefictionnovels #biotechnology #nanotechnology #theoreticalphysics #physics #darkmatter #utopian #strongfemalelead https://www.instagram.com/p/Bo1bqokgeJT/?utm_source=ig_tumblr_share&igshid=98bv21jpi1jt


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8 years ago

Largest Batch of Earth-size, Habitable Zone Planets

Our Spitzer Space Telescope has revealed the first known system of seven Earth-size planets around a single star. Three of these planets are firmly located in an area called the habitable zone, where liquid water is most likely to exist on a rocky planet.

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This exoplanet system is called TRAPPIST-1, named for The Transiting Planets and Planetesimals Small Telescope (TRAPPIST) in Chile. In May 2016, researchers using TRAPPIST announced they had discovered three planets in the system.

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Assisted by several ground-based telescopes, Spitzer confirmed the existence of two of these planets and discovered five additional ones, increasing the number of known planets in the system to seven.

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This is the FIRST time three terrestrial planets have been found in the habitable zone of a star, and this is the FIRST time we have been able to measure both the masses and the radius for habitable zone Earth-sized planets.

All of these seven planets could have liquid water, key to life as we know it, under the right atmospheric conditions, but the chances are highest with the three in the habitable zone.

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At about 40 light-years (235 trillion miles) from Earth, the system of planets is relatively close to us, in the constellation Aquarius. Because they are located outside of our solar system, these planets are scientifically known as exoplanets. To clarify, exoplanets are planets outside our solar system that orbit a sun-like star.

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In this animation, you can see the planets orbiting the star, with the green area representing the famous habitable zone, defined as the range of distance to the star for which an Earth-like planet is the most likely to harbor abundant liquid water on its surface. Planets e, f and g fall in the habitable zone of the star.

Using Spitzer data, the team precisely measured the sizes of the seven planets and developed first estimates of the masses of six of them. The mass of the seventh and farthest exoplanet has not yet been estimated.

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For comparison…if our sun was the size of a basketball, the TRAPPIST-1 star would be the size of a golf ball.

Based on their densities, all of the TRAPPIST-1 planets are likely to be rocky. Further observations will not only help determine whether they are rich in water, but also possibly reveal whether any could have liquid water on their surfaces.

The sun at the center of this system is classified as an ultra-cool dwarf and is so cool that liquid water could survive on planets orbiting very close to it, closer than is possible on planets in our solar system. All seven of the TRAPPIST-1 planetary orbits are closer to their host star than Mercury is to our sun.

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 The planets also are very close to each other. How close? Well, if a person was standing on one of the planet’s surface, they could gaze up and potentially see geological features or clouds of neighboring worlds, which would sometimes appear larger than the moon in Earth’s sky.

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The planets may also be tidally-locked to their star, which means the same side of the planet is always facing the star, therefore each side is either perpetual day or night. This could mean they have weather patterns totally unlike those on Earth, such as strong wind blowing from the day side to the night side, and extreme temperature changes.

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Because most TRAPPIST-1 planets are likely to be rocky, and they are very close to one another, scientists view the Galilean moons of Jupiter – lo, Europa, Callisto, Ganymede – as good comparisons in our solar system. All of these moons are also tidally locked to Jupiter. The TRAPPIST-1 star is only slightly wider than Jupiter, yet much warmer. 

How Did the Spitzer Space Telescope Detect this System?

Spitzer, an infrared telescope that trails Earth as it orbits the sun, was well-suited for studying TRAPPIST-1 because the star glows brightest in infrared light, whose wavelengths are longer than the eye can see. Spitzer is uniquely positioned in its orbit to observe enough crossing (aka transits) of the planets in front of the host star to reveal the complex architecture of the system. 

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Every time a planet passes by, or transits, a star, it blocks out some light. Spitzer measured the dips in light and based on how big the dip, you can determine the size of the planet. The timing of the transits tells you how long it takes for the planet to orbit the star.

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The TRAPPIST-1 system provides one of the best opportunities in the next decade to study the atmospheres around Earth-size planets. Spitzer, Hubble and Kepler will help astronomers plan for follow-up studies using our upcoming James Webb Space Telescope, launching in 2018. With much greater sensitivity, Webb will be able to detect the chemical fingerprints of water, methane, oxygen, ozone and other components of a planet’s atmosphere.

At 40 light-years away, humans won’t be visiting this system in person anytime soon…that said…this poster can help us imagine what it would be like: 

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

6 years ago

Merry Christmas from FTB Pathway Publications

Please enjoy

Merry Christmas From FTB Pathway Publications

Matthew Opdyke @ Author Central

http://www.amazon.com/dp/0578430436

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8 years ago
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?
What’s The Largest Planet In The Universe?

What’s The Largest Planet In The Universe?

“Above a certain mass, the atoms inside large planets will begin to compress so severely that adding more mass will actually shrink your planet. This happens in our Solar System, explaining why Jupiter is three times Saturn’s mass, but only 20% physically larger. But many solar systems have planets made out of much lighter elements, without large, rocky cores inside.”

You might think that Jupiter is the largest planet in the Solar System because it’s the most massive, but that’s not quite right. If you kept adding mass to Saturn, it would get larger in size, but if you kept adding mass to Jupiter, it would shrink! For a given set of elements that your planet is made out of, there’s a maximum size it can reach, that’s somewhere in between the mass of Saturn and Jupiter in general. Our Solar System is on the dense side of things, meaning that we’ve discovered a large number of exoplanets out there that are approximately twice the physical size of Jupiter without becoming brown dwarfs or hydrogen-fusing stars. For worlds like WASP-17b, where we’ve measured both the radius and mass, we find that they’re only about half the mass of Jupiter, despite being double the size.

Come get the full scientific story, and some very informative and illustrative images with no more than 200 words, on today’s Mostly Mute Monday!

7 years ago
Challenge And Tragedy Comes To Everyone, It Does Not Discriminate Between Good Or Bad... Our Resolve

Challenge and tragedy comes to everyone, it does not discriminate between good or bad... Our resolve to overcome these challenges and tragedies while maintaining our kindness and compassion, our dignity and grace, our vision to see a broader perspective and our strength of character to persevere are how we should measure ourselves... Only judge others based on the level of kindness they demonstrate, no matter what life brings, but be kind and love no matter the burden or reward... - 💜 -- Matt Opdyke

5 years ago
Four Videos Here. 1. Vesha's Story (chill Version) 2 & 3. Eliza's Story (chill And The Other Rockin)

Four videos here. 1. Vesha's story (chill version) 2 & 3. Eliza's story (chill and the other rockin) 4. James' story (chill) Let me know what you think. There is a lot of behind the scenes artwork. Enjoy =) #scifiauthor #spaceopera #ebooks paperbacks #fantasy #astronomy #sciencefiction #pathwaytothestars #politicalsciencefiction #longevity #CRISPR #physiology #architect #neuroscience #physics #theoreticalphysics #biotechnology #nanotechnology #matthewjopdyke #philosophy #wellbeing #spacetravel #solarsystem #books https://www.instagram.com/p/B0c9BK0BAeZ/?igshid=1plgw1wv7lxj0


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7 years ago

Interesting facts about stars

Stars are giant, luminous spheres of plasma. There are billions of them — including our own sun — in the Milky Way Galaxy. And there are billions of galaxies in the universe. So far, we have learned that hundreds also have planets orbiting them.

1. Stars are made of the same stuff

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All stars begin from clouds of cold molecular hydrogen that gravitationally collapse. As they cloud collapses, it fragments into many pieces that will go on to form individual stars. The material collects into a ball that continues to collapse under its own gravity until it can ignite nuclear fusion at its core. This initial gas was formed during the Big Bang, and is always about 74% hydrogen and 25% helium. Over time, stars convert some of their hydrogen into helium. That’s why our Sun’s ratio is more like 70% hydrogen and 29% helium. But all stars start out with ¾ hydrogen and ¼ helium, with other trace elements.

2. Most stars are red dwarfs

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If you could collect all the stars together and put them in piles, the biggest pile, by far, would be the red dwarfs. These are stars with less than 50% the mass of the Sun. Red dwarfs can even be as small as 7.5% the mass of the Sun. Below that point, the star doesn’t have the gravitational pressure to raise the temperature inside its core to begin nuclear fusion. Those are called brown dwarfs, or failed stars. Red dwarfs burn with less than 1/10,000th the energy of the Sun, and can sip away at their fuel for 10 trillion years before running out of hydrogen.

3. Mass = temperature = color

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The color of stars can range from red to white to blue. Red is the coolest color; that’s a star with less than 3,500 Kelvin. Stars like our Sun are yellowish white and average around 6,000 Kelvin. The hottest stars are blue, which corresponds to surface temperatures above 12,000 Kelvin. So the temperature and color of a star are connected. Mass defines the temperature of a star. The more mass you have, the larger the star’s core is going to be, and the more nuclear fusion can be done at its core. This means that more energy reaches the surface of the star and increases its temperature. There’s a tricky exception to this: red giants. A typical red giant star can have the mass of our Sun, and would have been a white star all of its life. But as it nears the end of its life it increases in luminosity by a factor of 1000, and so it seems abnormally bright. But a blue giant star is just big, massive and hot.

4. Most stars come in multiples

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It might look like all the stars are out there, all by themselves, but many come in pairs. These are binary stars, where two stars orbit a common center of gravity. And there are other systems out there with 3, 4 and even more stars. Just think of the beautiful sunrises you’d experience waking up on a world with 4 stars around it.

5. The biggest stars would engulf Saturn

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Speaking of red giants, or in this case, red supergiants, there are some monster stars out there that really make our Sun look small. A familiar red supergiant is the star Betelgeuse in the constellation Orion. It has about 20 times the mass of the Sun, but it’s 1,000 times larger. But that’s nothing. The largest known star is the monster UY Scuti.  It is a current and leading candidate for being the largest known star by radius and is also one of the most luminous of its kind. It has an estimated radius of 1,708 solar radii (1.188×109 kilometres; 7.94 astronomical units); thus a volume nearly 5 billion times that of the Sun.

6. There are many, many stars

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Quick, how many stars are there in the Milky Way. You might be surprised to know that there are 200-400 billion stars in our galaxy. Each one is a separate island in space, perhaps with planets, and some may even have life.

7. The Sun is the closest star

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Okay, this one you should know, but it’s pretty amazing to think that our own Sun, located a mere 150 million km away is average example of all the stars in the Universe. Our own Sun is classified as a G2 yellow dwarf star in the main sequence phase of its life. The Sun has been happily converting hydrogen into helium at its core for 4.5 billion years, and will likely continue doing so for another 7+ billion years. When the Sun runs out of fuel, it will become a red giant, bloating up many times its current size. As it expands, the Sun will consume Mercury, Venus and probably even Earth. 

8. The biggest stars die early

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Small stars like red dwarfs can live for trillions of years. But hypergiant stars, die early, because they burn their fuel quickly and become supernovae. On average, they live only a few tens of millions of years or less.

9. Failed stars

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Brown dwarfs are substellar objects that occupy the mass range between the heaviest gas giant planets and the lightest stars, of approximately 13 to 75–80 Jupiter masses (MJ). Below this range are the sub-brown dwarfs, and above it are the lightest red dwarfs (M9 V). Unlike the stars in the main-sequence, brown dwarfs are not massive enough to sustain nuclear fusion of ordinary hydrogen (1H) to helium in their cores.

10. Sirius: The Brightest Star in the Night Sky

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Sirius is a star system and the brightest star in the Earth’s night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The system has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is a binary star system, consisting of a white main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. 

To know more click the links: white dwarf, supernova, +stars, pulsars

sources: wikipedia and universetoday.com

image credits: NASA/JPL, Morgan Keenan, ESO, Philip Park / CC BY-SA 3.0

5 years ago

Lauge - Ephemeral Flower (Cloud Garden Mix) [SpaceAmbient]


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5 years ago
(I Got A Little Artsy For The Promo Videos And Wanted To Share...) PATHWAY TO THE STARS: PART 2, ELIZA

(I got a little artsy for the promo videos and wanted to share...) PATHWAY TO THE STARS: PART 2, ELIZA WILLIAMS is the second in the space opera booklet series, PATHWAY TO THE STARS. "We need to understand how dark energy and dark matter work, find ways to slow down the expansion or cause the Universe to breathe just enough to protect itself and all of life along with it. We need everyone who is willing." ~ Yesha Alevtina talking with Eliza Williams The story continues, Experience the early life of our future scientific and political hero, Eliza Williams, and the beginning of a new era! Vesha Celeste continues her training and journey with Yesha Alevtina, who shows and teaches her about Eliza Williams, through complete experiential immersion in the Virtual Universe. With the added advantages of time-dilation, neural linking, and nano-technology giving her tactile-reference, she sees Eliza’s life as if she were Eliza, herself. Vesha witnesses the critical aspects that lead to Eliza’s transformation and the formation of Pathway LLC. Eliza’s work to create the first biopods for physiological and neurological optimizations will be one of her primary vehicles to drive all of her advances and designs, solar-system-wide. There is a lot for Vesha to learn, and she too will play an integral role in our journeys throughout the cosmos, as this story progresses. Each ability she experiences in others, her optimized mind will be capable of learning and expounding upon exponentially. Enjoy the second part of this space opera booklet series, as we see our team of heroes doing what they can to help humanity in their quest to save the Universe one very-important step at a time. Enjoy this continuing saga as we are introduced to Eliza Williams, a critical leader-in-the-making, in this pathway to the stars! Available in paperback on Amazon Kindle and Barnes & Noble online. eBook available for $2.99 via Kindle eBooks. Audiobook is in the works, narrated and produced by Allison Taylor. #spaceopera #spaceoperabooks #scifibooks #scifi #fantasy #books #solarsystem #CRISPR #neuroscience #longevity #wellbeingfirst #pathwaytothestars https://www.instagram.com/p/B1YlbtWhFxK/?igshid=lovyil9nitpj


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5 years ago
To All Women, Who Dedicate Hours On End Toward Helping Others With Little Thought Of Reward In Return

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

matthewjopdyke - Matthew J. Opdyke
Matthew J. Opdyke

Author Matthew J. Opdyke, Science Fiction and Fantasy

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