He Always Fell For Puppies.

This is why you should always speak your mind

I made the top comment on the Star Wars Facebook, criticizing the Benioff and Weiss hire.

I present: comments from three hundred upset men (and women!) and why none of them have shaken my belief in how bad a hire this is.

I knew my remark would be unpopular and met with nasty comments, misguided statements about Game of Thrones and the film industry, insinuations that there aren’t any good women or nonwhite directions, couple of lewd comments about my sex life. There is truth to the adage: Facebook is a cesspool.

What I didn’t know is that I would get enough attention to make the top comment.

At the time of writing, sixty hours after initial posting, it’s running a little less than 80% laugh reactions—so, people thinking I’m a moron—and it’s running about 1,100 reactions and 324 replies.

Unfortunately for my would-be adversaries, I don’t debate on Facebook and it is a favorite pastime to read the vitriol and mediocre hash slung in my direction as if it’ll have any effect on my self-esteem. Fortunately, you don’t have to do the same. I present: the major response patterns and why they don’t hold any water.

Some basic science 🤓

Astronomy and Astrophysics: Facts

Here is a list of some curiosities of astronomy and astrophysics. From our solar system to interstellar space.

Mercury is shrinking: It’s small, it’s hot and it’s shrinking. A NASA-funded research suggests that Mercury is still contracting today, joining Earth as a tectonically active planet.

Stellar neighbor:  Proxima Centauri is a red dwarf, a small low-mass star, about 4.25 light-years (1.30 pc) from the Sun in the constellation of Centaurus. Proxima Centauri is the nearest star of the Sun that is known and at first can only be seen from the Southern Hemisphere.

A heavy star:  5 milliliters, or one teaspoon of neutron star material, equals the weight of about 900 Great Pyramids of Giza. One sugar cube equates to 100 billion tons. A cubic meter? The entire weight of the Atlantic Ocean. With an escape velocity of 100,000 km/s (Earth’s is a puny 11.3 km/s), a fall from 1 meter above a neutron star would only take one microsecond, and you would impact at around 2000 km/s, or 7.2 million kilometers per hour. This force would destroy all your component atoms, rendering all your matter identical. Fortunately, the closest neutron star is rather far away (about 400 light-years), so I wouldn’t be too concerned about the aforementioned event.

Asteroid belt: The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets.  About half the mass of the belt is contained in the four largest asteroids: Ceres, Vesta, Pallas, and Hygiea. The total mass of the asteroid belt is approximately 4% that of the Moon, or 22% that of Pluto, and roughly twice that of Pluto’s moon Charon (whose diameter is 1200 km).

Sunlight Takes Around 8 Minutes To Reach Earth: The Earth is located 93 million miles (150 million kms) away from the Sun, a distance known to astronomers as an astronomical units or AU. Traveling at the speed of light (186,282 miles per second), sunlight is able to cross this vast distance in around 8 minutes 20 seconds.

Pluto is about 2,376 km in diameter. Pluto’s small size and low mass mean that it has a density of 1.86 grams per cubic centimeter according to recent measurements by New Horizons, about 40 percent of Earth’s density.

Just like black holes; neutron stars also generate gravitational waves: This year astronomers were able to detect gravitational waves originating from neutron stars. And in addition, it was possible to observe the location of the collision thanks to the efforts of the astronomers. This is a great advance for astronomy.

Most neutron stars are very fast rotators: Since the conservation of angular momentum following a supernova explosion transfers the progenitor star’s rate of rotation to the remnant that is only about 20 km (12.5 miles) in diameter, the result is that the neutron star rotates very rapidly when it is formed. Most known neutron stars rotate several hundred times per second, but the fastest rotator yet discovered, the neutron star designated PSR J1748-2446ad, is known to rotate 716 times per second, which translates into 43,000 rotations per minute, or 24% of the speed of light at the star’s equatorial surface.

Asteroid also has satellite: This color picture is made from images taken by the imaging system on the Galileo spacecraft about 14 minutes before its closest approach to asteroid 243 Ida on August 28, 1993. Ida’s moon, Dactyl, was discovered by mission member Ann Harch in images returned from Galileo. It was named after the Dactyls, creatures which inhabited Mount Ida in Greek mythology. Ida has an average diameter of 31.4 km (19.5 mi). It is irregularly shaped and elongated, and apparently composed of two large objects connected together. Its surface is one of the most heavily cratered in the Solar System, featuring a wide variety of crater sizes and ages.

Kepler-444 system: The oldest known planetary system has five terrestrial-sized planets, all in orbital resonance. This weird group showed that solar systems have formed and lived in our galaxy for nearly its entire existence. Estimated to be 11.2 billion years old (more than 80% of the age of the universe), approximately 117 light-years (36 pc) away from Earth in the constellation Lyra. 

Sources: wikipedia, space.com, futurism.com and astronomytrek.com

Image credit: NASA/JPL, ESO/M. Kornmesser, NASA/XMM Newton, Casey Reed/Penn State University, NASA/ESA/Hubble

To learn more about the shrinkage of Mercury, click here.

To learn more about the gravitational waves generated by neutron stars click here.

Neil 2020

8.28.17

I love this

Rachel C Lewis | @wnq-quoteoftheday | @wordsnquotes-online

The future is kelp

The push for renewable energy in the U.S. often focuses on well-established sources of electricity: solar, wind and hydropower. Off the coast of California, a team of researchers is working on what they hope will become an energy source of the future — macroalgae, otherwise known as kelp.

The Pacific Coast is known for its vast kelp forests. It’s one of the fastest-growing plants on Earth, and farming it requires no fertilizer, fresh water, pesticides, or arable land. “It can grow 2 to 3 feet per day,” says Diane Kim, one of the scientists running the kelp research project at the University of Southern California.

Kelp is transformed into biofuel by a process called thermochemical liquefaction. The kelp is dried out, and the salt is washed away. Then it’s turned into bio-oil through a high-temperature, high-pressure conversion process.

Some small companies are growing kelp as a substitute for kale in the U.S., but that’s exactly the problem – very, very few are doing it. Thus, the infrastructure and investment isn’t in place to make other products from kelp, like biofuel.

Scientists Hope To Farm The Biofuel Of The Future In The Pacific Ocean

Photos: Courtesy of David Ginsburg/Wrigley Institute, Monika Evstatieva/NPR (2) and Anjuli Sastry/NPR

I believe

The X-Files Season 11 - 90s print ads inspired

pls credit if you repost.

I’m so mad that a t4 bacteriophage actually looks like that and that it’s appearance isn’t made up

a brief departure from the typical posts here…

while i try not to include my personal work in subtilitas, readers may have noticed content has been a little sparse here lately, largely due to a few large projects wrapping up. one of which is a book i’ve been involved with through the cactus store, which was just released this week.

xerophile is a compendium of desert plant and habitat photography three years in the making. a selection of over five hundred photographs of arguably the rarest and most bizarre plants on earth, photographed in their remote natural habitats over the past 80 years by a global cadre of obsessed cactus aficionados made up of both the amateur and the professional—from phd. botanist to banker, art teacher to cancer researcher. aside from the field photography, we’ve also included several interviews with the explorer’s themselves, who’s stories only add to the mystique of their images. 

posts should begin to be more regular next week. thanks as always for reading.

I want to live with SOFIA in the sky

What's Inside SOFIA? High Flying Instruments

Our flying observatory, called SOFIA, carries a 100-inch telescope inside a Boeing 747SP aircraft. Having an airborne observatory provides many benefits.

It flies at 38,000-45,000 feet – above 99% of the water vapor in Earth’s atmosphere that blocks infrared light from reaching the ground! 

It is also mobile! We can fly to the best vantage point for viewing the cosmos. We go to Christchurch, New Zealand, nearly every year to study objects best observed from the Southern Hemisphere. And last year we went to Daytona Beach, FL, to study the atmosphere of Neptune’s moon Triton while flying over the Atlantic Ocean.

SOFIA’s telescope has a large primary mirror – about the same size as the Hubble Space Telescope’s mirror. Large telescopes let us gather a lot of light to make high-resolution images!

But unlike a space-based observatory, SOFIA returns to our base every morning.

Which means that we can change the instruments we use to analyze the light from the telescope to make many different types of scientific observations. We currently have seven instruments, and new ones are now being developed to incorporate new technologies.

So what is inside SOFIA? The existing instruments include:

Infrared cameras that can peer inside celestial clouds of dust and gas to see stars forming inside. They can also study molecules in a nebula that may offer clues to the building blocks of life…

…A polarimeter, a device that measures the alignment of incoming light waves, that we use to study magnetic fields. The left image reveals that hot dust in the starburst galaxy M82 is magnetically aligned with the gas flowing out of it, shown in blue on the right image from our Chandra X-ray Observatory. This can help us understand how magnetic fields affect how stars form.

…A tracking camera that we used to study New Horizon’s post-Pluto flyby target and found that it may have its own moon…

…A spectrograph that spreads light into its component colors. We’re using one to search for signs of water plumes on Jupiter’s icy moon Europa and to search for signs of water on Venus to learn about how it lost its oceans…

…An instrument that studies high energy terahertz radiation with 14 detectors. It’s so efficient that we made this map of Orion’s Horsehead Nebula in only four hours! The map is made of 100 separate views of the nebula, each mapping carbon atoms at different velocities.

…And we have an instrument under construction that will soon let us study how water vapor, ice and oxygen combine at different times during planet formation, to better understand how these elements combine with dust to form a mass that can become a planet.

Our airborne telescope has already revealed so much about the universe around us! Now we’re looking for the next idea to help us use SOFIA in even more new ways. 

Discover more about our SOFIA flying observatory HERE. 

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