Planetary Nebula IC 4406 In The Constellation Lupus

A shot of just a tiny bit of the Andromeda Galaxy, from the sharpest ever view taken by the Hubble Space Telescope

Full size image

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.

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.

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.

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.

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.

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.

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.

 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.

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.

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. 

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.

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: 

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

How to Escape a Hair Grab or a Neck Grab ? Look at them, carefully.

tai chi pants on http://www.icnbuys.com/tai-chi-pants give you surprise at the new year.

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Saturn’s hexagon

This colorful view from NASA’s Cassini mission is the highest-resolution view of the unique six-sided jet stream at Saturn’s north pole known as “the hexagon.” This movie, made from images obtained by Cassini’s imaging cameras, is the first to show the hexagon in color filters, and the first movie to show a complete view from the north pole down to about 70 degrees north latitude.

Via NASA: In Full View: Saturn’s Streaming Hexagon

On October 8 a privileged few could see auroras in abnormally low latitudes, as the spectacular pictures above taken in Wales and Northern England.

Via TON: Northern Lights Put On Spectacular Show As Aurora Borealis Lit Skies Over Wales And Yorkshire.

SwRI’s Parker discovers moon over Makemake in the Kuiper Belt A Southwest Research Institute-led team has discovered an elusive, dark moon orbiting Makemake, one of the “big four” dwarf planets populating the Kuiper Belt region at the edge of our solar system. The findings are detailed in the paper “Discovery of a Makemakean Moon,” published in the June 27 issue of Astrophysical Journal Letters.

“Makemake’s moon proves that there are still wild things waiting to be discovered, even in places people have already looked,” said Dr. Alex Parker, lead author of the paper and the SwRI astronomer credited with discovering the satellite. Parker spotted a faint point of light close to the dwarf planet using data from Hubble’s Wide Field Camera 3. “Makemake’s moon – nicknamed MK2 – is very dark, 1,300 times fainter than the dwarf planet.”

A nearly edge-on orbital configuration helped it evade detection, placing it deep within the glare of the icy dwarf during a substantial fraction of its orbit. Makemake is one of the largest and brightest known Kuiper Belt Objects (KBOs), second only to Pluto. The moon is likely less than 100 miles wide while its parent dwarf planet is about 870 miles across. Discovered in 2005, Makemake is shaped like football and sheathed in frozen methane.

“With a moon, we can calculate Makemake’s mass and density,” Parker said. “We can contrast the orbits and properties of the parent dwarf and its moon, to understand the origin and history of the system. We can compare Makemake and its moon to other systems, and broaden our understanding of the processes that shaped the evolution of our solar system.”

With the discovery of MK2, all four of the currently designated dwarf planets are known to host one or more satellites. The fact that Makemake’s satellite went unseen despite previous searches suggests that other large KBOs may host hidden moons.

Prior to this discovery, the lack of a satellite for Makemake suggested that it had escaped a past giant impact. Now, scientists will be looking at its density to determine if it was formed by a giant collision or if it was grabbed by the parent dwarf’s gravity. The apparent ubiquity of moons orbiting KBO dwarf planets supports the idea that giant collisions are a near-universal fixture in the histories of these distant worlds.

top Image: illustration shows Makemake’s bright red surface and the inferred darker surface of the moon, known as MK2. Image Courtesy of NASA/SwRI/Alex Parker

lower Image: Different views of the Makemake system taken two days apart. Image Courtesy of NASA/Hubble WFC3/SwRI/Alex Parker

Some websites that I use for geography [lessons + revision] - a mix of summary notes websites, statistics, geo-located data and other goodies :D enjoy! Hope you find something useful! 

I’ve only put my faves tbh but ** = I’ve used this a lot A LOT 

Scribd: honestly some docs on here are so useful for help structuring your own notes etc. [our teacher uses this one for example for the glossary]

**Sporcle: i use this to test my place knowledge! [i’ve linked you to the world one, but you can find other continent specific ones too]

[Alternative to above that I personally haven’t used much but it looks decent so]

World Mapper: Really cool maps and omg countries look so funny distorted heu heu (HONESTLY SO USEFUL AND VISUAL) [i’ve linked to the old site haha]

**Gapminder: I’ve linked you to the program itself [so so so good omg for global trends over time GENIUS] but Hans Rosling is a cinnamon roll go watch the videos too!!

Information is beautiful: I love infographics okay fight me on this. You could have a look at this one and oh here’s the blog and just have an explore tbh [there’s isn’t a huge number of infographics on here tbh it’s a shame but i guess they’re trying to sell the book so fair]

**Datashine (UK centric): UK Census 2011 info geo-located and ahhh it’s so useful 

they also have this one on commuting if you’re about that life

*******CIA World Factbook: ALL THE STATS! LIFESAVER! 10Q America! (that maths pun stop me pls) 

Generally amazing website that is succinct and you could probably find so much on here tbh

Quizlet: really useful resource!! flashcards!! i love this site!! (and there’s an app hehe) test yourself on case studies etc!!

[tip: you can duplicate ppl’s flashcards and edit them if there’s anything you want to add!] 

BBC bitesize ayyy for gcse peeps! (and in general too :) ) 

S-cool [linked again to the gcse site cuz that’s what was bookmarked but they have an a-level section too!] Some real concise notes tbh and may be useful even if you aren’t studying gcses/alevels! :) 

my other masterpost/ramble hybrids are all (there’s like 2 others lol) here and feel free to come rant at me (or just talk lel) if any links don’t work etc! 

in hindsight a better header for this would have been ‘resources i rely on way too much for geography’ (*´◡`) 

is there anything you can tell us to expand on the space time ripples found in simulated black hole collisions?

Hi!

In one of my other responses I explained the whole concept of space time, here’s how i explained that:

A way that you can picture the bending of space time is this:

Picture two chairs, the backs facing each other. Then tape one end of a blanket to one of the chair backs and the other end of the blanket to the other chair back. What you have now should like this:

Now, if you were to place a tennis ball somewhere on the light blue blanket (top blanket), that blanket would no longer be flat, there would be a bend or a curve in it. Let’s say you put a basketball on the top blanket instead of a tennis ball. Since the basketball is bigger, the bend/curve that it makes will be a lot bigger than the tennis ball’s because the basketball has more mass.

So that blue blanket at the top of the chairs represents space time. If there were to be two large objects, let’s say basketballs, that were to “collide” (representing two black holes). Since they’re so large, they’d create these ripples in the blanket that can be observed.

Another easier way to think about it is like dropping a pebble into a lake. The bigger the pebble, the stronger and more frequent the ripples are. So since black holes are very massive, they create larger ripples compared to something smaller!

Astronomers haven’t been able to directly observe these ripples in space time, they were theorized by Einstein, however there’s an announcement being made all over the world today about data obtained from the Laser Interferometer Gravitational-Wave Observatory (LIGO)!

Here is a link talking a bit about that press conference!

I hope that helped to clarify everything! If not, feel free to ask again and I’ll try my best to clarify!

UPDATE: HERE are the findings of the conference, they’ve detected them for the first time!

Helix nebula

js

Behold NGC 6357, “cathedral to massive stars.” Credit: NASA, ESA and Jesús Maíz Apellániz (IAA, Spain). (NASA/APOD)