The 4th dimension in our case is where the 3D structures including this very Universe combine and exist within changing time frames. 4D structures can’t exist within 3D ones but 3D structures can exist in a 4D just like your drawings exist within that flat paper as lines and points but couldn’t exist in our 3D world by itself. Extra dimensions work the same, like a Matryoshka doll that loses and or gains properties the further you go.

Image: 3D projection of a tesseract undergoing a simple rotation in four dimensional space.

In mathematical physics, Minkowski space or Minkowski spacetime (named after the mathematician Hermann Minkowski) is the mathematical space setting in which Einstein’s theory of special relativity is most conveniently formulated. In this setting the three ordinary dimensions of space are combined with a single dimension of time to form a four-dimensional manifold for representing a spacetime. [**]

In physics, spacetime (also space–time, space time or space–time continuum) is any mathematical model that combines space and time into a single continuum. Spacetime is usually interpreted with space as existing in three dimensions and time playing the role of a fourth dimension that is of a different sort from the spatial dimensions. From a Euclidean space perspective, the universe has three dimensions of space and one of time. By combining space and time into a single manifold, physicists have significantly simplified a large number of physical theories, as well as described in a more uniform way the workings of the universe at both the supergalactic and subatomic levels. [**]

But my favorite explanation of extra dimensions in general is Carl Sagan’s version. His version was based on Flatland: A Romance of Many Dimensions which is an 1884 satirical short story by Edwin Abbott Abbott:

The story is about a two-dimensional world referred to as Flatland which is occupied by geometric figures. Women are simple line-segments, while men are polygons with various numbers of sides. The narrator is a humble square, a member of the social caste of gentlemen and professionals in a society of geometric figures, who guides us through some of the implications of life in two dimensions. The Square has a dream about a visit to a one-dimensional world (Lineland) which is inhabited by “lustrous points”.

He attempts to convince the realm’s ignorant monarch of a second dimension but finds that it is essentially impossible to make him see outside of his eternally straight line.

He is then visited by a three-dimensional sphere, which he cannot comprehend until he sees Spaceland for himself. This Sphere (who remains nameless, like all characters in the novella) visits Flatland at the turn of each millennium to introduce a new apostle to the idea of a third dimension in the hopes of eventually educating the population of Flatland of the existence of Spaceland. From the safety of Spaceland, they are able to observe the leaders of Flatland secretly acknowledging the existence of the sphere and prescribing the silencing of anyone found preaching the truth of Spaceland and the third dimension. After this proclamation is made, many witnesses are massacred or imprisoned (according to caste).

After the Square’s mind is opened to new dimensions, he tries to convince the Sphere of the theoretical possibility of the existence of a fourth (and fifth, and sixth …) spatial dimension.

The depiction above is a 4 dimensional figure as represented by 3 dimensional cubes within cubes to visualize how 4th dimensions may work.

Related: Carl Sagan explains extra dimensions

Galaxy Collisions: Simulation vs Observations

The folks over at NASA apod just put up an awesome galaxy collisions, simulations and observations video for the public. I made a little gif set to go along with the video which can be found here.

What happens when two galaxies collide? Although it may take over a billion years, such titanic clashes are quite common.

Images Credit: NASA, ESA; Visualization: Frank Summers (STScI);

Simulation: Chris Mihos (CWRU) & Lars Hernquist (Harvard).

Since galaxies are mostly empty space, no internal stars are likely to themselves collide. Rather the gravitation of each galaxy will distort or destroy the other galaxy, and the galaxies may eventually merge to form a single larger galaxy.

Expansive das and dust clouds collide and trigger waves of star formation that complete even during the interaction process. Pictured above is a computer simulation of two large spiral galaxies colliding, interspersed with real still images taken by the Hubble Space Telescope.

Our own Milky Way Galaxy has absorbed several smaller galaxies during its existence and is even projected to merge with the larger neighboring Andromeda galaxy in a few billion years.

Dances from Around the World: Children learn to program using KIWI robots

A robotics curricular unit integrating themes of dance, music, and culture with engineering, building, and programming. A research project directed Professor Marina Umaschi Bers at the DevTech Research Group at Tufts University.

The KIWI robotics construction set is designed to work with CHERP software (Creative Hybrid Environment for Robotic Programming). CHERP is a hybrid tangible/graphical computer language designed to provide an engaging introduction to computer programming for children in both formal and informal educational settings. CHERP was designed at Tufts University by the DevTech Research Group (NSF Grant No. DRL-0735657).

(Ready For Robotics)

"To be clear, I do not have a problem with increased protection or security. Who’s to say that a shooting won’t occur at the next student party? It could happen, God forbid, and I understand why USC wants to be prepared. My issue lies within the selective surveillance of minority-hosted parties, as if crimes only happen among high concentrations of melanin. Hundreds of criminal offenses, including sexual harassment, rape and assault happen every Thursday night on Greek Row, a undeniably white establishment. Yet, the culprits of the Department of Public Safety Crime Reports distributed to USC students and faculty, seem to be strictly limited to Black and Latino males (6’2-6’5 in dark hoodies)."

blackcyborgs:

I’m a Scholar, Not a Criminal: The Plight of Black Students at USC
Instead of studying for the last final of my undergraduate career, I am writing this letter in protest of the University of Southern California’s latest atrocity. Last night, students gathered at a house near campus to celebrate their completion of another rigorous school year. Many attendees were graduating seniors. Almost all attendees were minority students: African-American and Latino.
I did not attend last night’s party, but I could hear the helicopter circling from my dorm room over a mile away. When the Facebook posts and photos started appearing on my news feed around 2:30am, I had flashbacks to an era I wasn’t even alive to suffer through. I was too scared to go outside, legitimately fearing that an officer would see me and arrest me for being Black and inquisitive. I can only imagine how my peers felt when they saw over twenty LAPD patrol cars pull up and release 79 officers to end a peaceful, congratulatory party.
It is inexpressibly disheartening to hear fellow students recount horror stories of police brutality two weeks away from being among the first in my family to graduate from a four-year university. To know that my college degree holds no weight in the face of institutional racism and discrimination is sobering. Since the three most recent shootings, all triggered by non-USC affiliated Black males, that occurred on and around USC, there has been an increased presence of LAPD and other security forces around campus. Amid the tense racial climate that followed, I patiently endured the ignorant comments, racist blog posts and suspicious stares, but the intolerance has reached a new high. Six of my friends spent the night in jail.
To be clear, I do not have a problem with increased protection or security. Who’s to say that a shooting won’t occur at the next student party? It could happen, God forbid, and I understand why USC wants to be prepared. My issue lies within the selective surveillance of minority-hosted parties, as if crimes only happen among high concentrations of melanin. Hundreds of criminal offenses, including sexual harassment, rape and assault happen every Thursday night on Greek Row, a undeniably white establishment. Yet, the culprits of the Department of Public Safety Crime Reports distributed to USC students and faculty, seem to be strictly limited to Black and Latino males (6’2-6’5 in dark hoodies). These reports, together with the newly constructed, other-izing gates around campus, have instilled an unhealthy amount of fear in students, administrators and safety officials. We have been trained to double check for USC logos on the sweatshirts of minority males on and around this campus to make sure that they’re “one of us.” It doesn’t surprise me that LAPD has adopted the same attitude. For them, it has been this way for decades.
If the USC Department of Public Safety feels justified in allowing nearly a hundred police officers to shut down a minority attended party due to the fact that African-Americans were responsible for the recent shootings, we’re in for a bigger battle than most students bargained for when they decided to enroll here. That ideology reeks of racial profiling and associates the behavior of a few criminals with the entire Black student body, a comparison that makes my stomach turn. While LAPD is busy sending all of their manpower to harass the future of America’s leaders, the real trouble lies within my campus’ freshly painted fences.
USC should not be permitted to reap the benefits of diversity without facing its complexities. You can’t help the hood without loving it first. When USC’s founders decided to break ground in South Central instead of Malibu, it signed up for a difficult and delicate community partnership that needs to be revisited.
To me, protection means opening our gates even wider for at-risk youth who are in desperate need of positive role models, not locking them out after 9pm. I will feel safe on this campus when I see DPS officers negotiating with LAPD, pleading with them to let students of color party in peace. I will feel welcomed when I see a public statement from President Nikias acknowledging the discrimination and blatant racism that my people have had to endure since we were first admitted into this school. I will become a proud Trojan when the USC community finally grows to reflect and embrace its resilient surroundings.
To my peers, I am sorry that we have to dedicate hours that should be spent studying to defend our freedom of assembly. None of us have the time to write letters, plan meetings and rally against injustice, but we must. The next generation of brilliant Black students is depending on us to guarantee their right to a dignified college experience.
Ways to Act:
Sign this petition to help end racial profiling at USC: http://www.change.org/petitions/stop-racial-profiling-at-usc
Attend the Sit-In at Tommy Trojan on Monday, May 6 from 12-4pm
Attend the DPS & LAPD Campus Discussion on Tuesday, May 7 at 6pm in Annenberg 204
*Meet in front of Annenberg at 5:30pm to pray over the meeting.

blackcyborgs:

I’m a Scholar, Not a Criminal: The Plight of Black Students at USC

Instead of studying for the last final of my undergraduate career, I am writing this letter in protest of the University of Southern California’s latest atrocity. Last night, students gathered at a house near campus to celebrate their completion of another rigorous school year. Many attendees were graduating seniors. Almost all attendees were minority students: African-American and Latino.

I did not attend last night’s party, but I could hear the helicopter circling from my dorm room over a mile away. When the Facebook posts and photos started appearing on my news feed around 2:30am, I had flashbacks to an era I wasn’t even alive to suffer through. I was too scared to go outside, legitimately fearing that an officer would see me and arrest me for being Black and inquisitive. I can only imagine how my peers felt when they saw over twenty LAPD patrol cars pull up and release 79 officers to end a peaceful, congratulatory party.

It is inexpressibly disheartening to hear fellow students recount horror stories of police brutality two weeks away from being among the first in my family to graduate from a four-year university. To know that my college degree holds no weight in the face of institutional racism and discrimination is sobering. Since the three most recent shootings, all triggered by non-USC affiliated Black males, that occurred on and around USC, there has been an increased presence of LAPD and other security forces around campus. Amid the tense racial climate that followed, I patiently endured the ignorant comments, racist blog posts and suspicious stares, but the intolerance has reached a new high. Six of my friends spent the night in jail.

To be clear, I do not have a problem with increased protection or security. Who’s to say that a shooting won’t occur at the next student party? It could happen, God forbid, and I understand why USC wants to be prepared. My issue lies within the selective surveillance of minority-hosted parties, as if crimes only happen among high concentrations of melanin. Hundreds of criminal offenses, including sexual harassment, rape and assault happen every Thursday night on Greek Row, a undeniably white establishment. Yet, the culprits of the Department of Public Safety Crime Reports distributed to USC students and faculty, seem to be strictly limited to Black and Latino males (6’2-6’5 in dark hoodies). These reports, together with the newly constructed, other-izing gates around campus, have instilled an unhealthy amount of fear in students, administrators and safety officials. We have been trained to double check for USC logos on the sweatshirts of minority males on and around this campus to make sure that they’re “one of us.” It doesn’t surprise me that LAPD has adopted the same attitude. For them, it has been this way for decades.

If the USC Department of Public Safety feels justified in allowing nearly a hundred police officers to shut down a minority attended party due to the fact that African-Americans were responsible for the recent shootings, we’re in for a bigger battle than most students bargained for when they decided to enroll here. That ideology reeks of racial profiling and associates the behavior of a few criminals with the entire Black student body, a comparison that makes my stomach turn. While LAPD is busy sending all of their manpower to harass the future of America’s leaders, the real trouble lies within my campus’ freshly painted fences.

USC should not be permitted to reap the benefits of diversity without facing its complexities. You can’t help the hood without loving it first. When USC’s founders decided to break ground in South Central instead of Malibu, it signed up for a difficult and delicate community partnership that needs to be revisited.

To me, protection means opening our gates even wider for at-risk youth who are in desperate need of positive role models, not locking them out after 9pm. I will feel safe on this campus when I see DPS officers negotiating with LAPD, pleading with them to let students of color party in peace. I will feel welcomed when I see a public statement from President Nikias acknowledging the discrimination and blatant racism that my people have had to endure since we were first admitted into this school. I will become a proud Trojan when the USC community finally grows to reflect and embrace its resilient surroundings.

To my peers, I am sorry that we have to dedicate hours that should be spent studying to defend our freedom of assembly. None of us have the time to write letters, plan meetings and rally against injustice, but we must. The next generation of brilliant Black students is depending on us to guarantee their right to a dignified college experience.

Ways to Act:

Sign this petition to help end racial profiling at USC: http://www.change.org/petitions/stop-racial-profiling-at-usc

Attend the Sit-In at Tommy Trojan on Monday, May 6 from 12-4pm

Attend the DPS & LAPD Campus Discussion on Tuesday, May 7 at 6pm in Annenberg 204

*Meet in front of Annenberg at 5:30pm to pray over the meeting.

The Current Types of Nebulae

Originally, the word “nebula” referred to almost any extended astronomical object (other than planets and comets). The etymological root of “nebula” means “cloud”. As is usual in astronomy, the old terminology survives in modern usage in sometimes confusing ways. We sometimes use the word “nebula” to refer to galaxies, various types of star clusters and various kinds of interstellar dust/gas clouds. More strictly speaking, the word “nebula” should be reserved for gas and dust clouds and not for groups of stars.

By order in which they appear from top to bottom, left to right, here are the main types and some provided examples for visual reference:

Planetary Nebulae: Sh2-188

Planetary nebulae are shells of gas thrown out by some stars near the end of their lives. Our Sun will probably evolve a planetary nebula in about 5 billion years. They have nothing at all to do with planets; the terminology was invented because they often look a little like planets in small telescopes. A typical planetary nebula is less than one light-year across.

Dark Nebulae: LDN 1622

Dark nebulae are clouds of dust which are simply blocking the light from whatever is behind. They are physically very similar to reflection nebulae; they look different only because of the geometry of the light source, the cloud and the Earth. Dark nebulae are also often seen in conjunction with reflection and emission nebulae. A typical diffuse nebula is a few hundred light-years across.

Emission Nebulae: NGC 896

Emission nebulae are clouds of high temperature gas. The atoms in the cloud are energized by ultraviolet light from a nearby star and emit radiation as they fall back into lower energy states (in much the same way as a neon light). These nebulae are usually red because the predominant emission line of hydrogen happens to be red (other colors are produced by other atoms, but hydrogen is by far the most abundant). Emission nebulae are usually the sites of recent and ongoing star formation.

Reflection Nebulae: NGC 1333

Reflection nebulae are clouds of dust which are simply reflecting the light of a nearby star or stars. Reflection nebulae are also usually sites of star formation. They are usually blue because the scattering is more efficient for blue light. Reflection nebulae and emission nebulae are often seen together and are sometimes both referred to as diffuse nebulae.

"Things like racism are institutionalized. You might not know any bigots. You feel like “well I don’t hate black people so I’m not a racist,” but you benefit from racism. Just by the merit, the color of your skin. The opportunities that you have, you’re privileged in ways that you might not even realize because you haven’t been deprived of certain things. We need to talk about these things in order for them to change."

Dave Chappelle

The Diamond Ring Effect

The Baily’s beads effect is a feature of total solar eclipses.

As the moon “grazes” by the Sun during a solar eclipse, the rugged lunar limb topography allows beads of sunlight to shine through in some places, and not in others. The name is in honor of Francis Baily who first provided an exact explanation of the phenomenon in 1836. The diamond ring effect is seen when only one bead is left; a shining diamond set in a bright ring around the lunar silhouette.

Chondrites and Chondrules


  Chondrites are stony meteorites. They’re the most common and probably the most fascinating type of meteorite. The meteor/meteorite that broke windows in the Russian city of Chelyabinsk this past February was a stony chondrite.
  
  The composition of chondrites is very similar to the composition of the Sun, except that they’re lacking hydrogen and helium. So, if you’d like to hold a piece of the Sun in your palm, chondrites are about as close as you can get. Their name is derived from the chondrules (spherical inclusions) observed in most of them. Chondrules are only found in meteorites.
  
  They’re over 4 billion years old — older than the Earth and other planets. Scientists previously identified meteorites by the crystals found within chondrules, but later they realized that chondrules may recrystallize during weathering processes once they reach the Earth’s surface. Sometimes a broken face of a meteorite is weathered in such a way that 3-D chondrules are seen (above at upper right corner). However, chrondules can be more easily studied by cutting the parent chrondite into slices. Shown at center is a a microscopic image of a 3 cm slice of a chondrite that was found in northwest Africa. — Mila Zinkova

Chondrites and Chondrules

Chondrites are stony meteorites. They’re the most common and probably the most fascinating type of meteorite. The meteor/meteorite that broke windows in the Russian city of Chelyabinsk this past February was a stony chondrite.

The composition of chondrites is very similar to the composition of the Sun, except that they’re lacking hydrogen and helium. So, if you’d like to hold a piece of the Sun in your palm, chondrites are about as close as you can get. Their name is derived from the chondrules (spherical inclusions) observed in most of them. Chondrules are only found in meteorites.

They’re over 4 billion years old — older than the Earth and other planets. Scientists previously identified meteorites by the crystals found within chondrules, but later they realized that chondrules may recrystallize during weathering processes once they reach the Earth’s surface. Sometimes a broken face of a meteorite is weathered in such a way that 3-D chondrules are seen (above at upper right corner). However, chrondules can be more easily studied by cutting the parent chrondite into slices. Shown at center is a a microscopic image of a 3 cm slice of a chondrite that was found in northwest Africa. — Mila Zinkova

Albert Einstein, Civil Rights Activist


  Here’s something you probably don’t know about Albert Einstein.
  
  Image:Einstein with the children of Lincoln University Faculty, May 3, 1946
  
  In 1946, the Nobel Prize-winning physicist traveled to Lincoln University in Pennsylvania, the alma mater of Langston Hughes and Thurgood Marshall and the first school in America to grant college degrees to blacks. At Lincoln, Einstein gave a speech in which he called racism “a disease of white people,” and added, “I do not intend to be quiet about it.” He also received an honorary degree and gave a lecture on relativity to Lincoln students.
  
  The reason Einstein’s visit to Lincoln is not better known is that it was virtually ignored by the mainstream press, which regularly covered Einstein’s speeches and activities. (Only the black press gave extensive coverage to the event.) Nor is there mention of the Lincoln visit in any of the major Einstein biographies or archives.
  
  In fact, many significant details are missing from the numerous studies of Einstein’s life and work, most of them having to do with Einstein’s opposition to racism and his relationships with African Americans.
  
  That these omissions need to be recognized and corrected is the contention of Fred Jerome and Rodger Taylor, authors of “Einstein on Race and Racism” (Rutgers University Press, 2006). Jerome and Taylor spoke April 3 at an event sponsored by the W.E.B. Du Bois Institute for African and African American Research. The event also featured remarks by Sylvester James Gates Jr., the John S. Toll Professor of Physics, University of Maryland.
  
  According to Jerome and Taylor, Einstein’s statements at Lincoln were by no means an isolated case. Einstein, who was Jewish, was sensitized to racism by the years of Nazi-inspired threats and harassment he suffered during his tenure at the University of Berlin. Einstein was in the United States when the Nazis came to power in 1933, and, fearful that a return to Germany would place him in mortal danger, he decided to stay, accepting a position at the recently founded Institute for Advanced Study in Princeton, N.J. He became an American citizen in 1940.
  
  But while Einstein may have been grateful to have found a safe haven, his gratitude did not prevent him from criticizing the ethical shortcomings of his new home.
  
  “Einstein realized that African Americans in Princeton were treated like Jews in Germany,” said Taylor. “The town was strictly segregated. There was no high school that blacks could go to until the 1940s.”
  
  Einstein’s response to the racism and segregation he found in Princeton (Paul Robeson, who was born in Princeton, called it “the northernmost town in the South”) was to cultivate relationships in the town’s African-American community. Jerome and Taylor interviewed members of that community who still remember the white-haired, disheveled figure of Einstein strolling through their streets, stopping to chat with the inhabitants, and handing out candy to local children.
  
  One woman remembered that Einstein paid the college tuition of a young man from the community. Another said that he invited Marian Anderson to stay at his home when the singer was refused a room at the Nassau Inn.
  
  Einstein met Paul Robeson when the famous singer and actor came to perform at Princeton’s McCarter Theatre in 1935. The two found they had much in common. Both were concerned about the rise of fascism, and both gave their support to efforts to defend the democratically elected government of Spain against the fascist forces of Francisco Franco. Einstein and Robeson also worked together on the American Crusade to End Lynching, in response to an upsurge in racial murders as black soldiers returned home in the aftermath of World War II.
  
  The 20-year friendship between Einstein and Robeson is another story that has not been told, Jerome said, but that omission may soon be rectified. A movie is in the works about the relationship, with Danny Glover slated to play Robeson and Ben Kingsley as Einstein.
  
  Einstein continued to support progressive causes through the 1950s, when the pressure of anti-Communist witch hunts made it dangerous to do so. Another example of Einstein using his prestige to help a prominent African American occurred in 1951, when the 83-year-old W.E.B. Du Bois, a founder of the NAACP, was indicted by the federal government for failing to register as a “foreign agent” as a consequence of circulating the pro-Soviet Stockholm Peace Petition. Einstein offered to appear as a character witness for Du Bois, which convinced the judge to drop the case.
  
  Gates, an African-American physicist who has appeared on the PBS show Nova, said that Einstein had been a hero of his since he learned about the theory of relativity as a teenager, but that he was unaware of Einstein’s ideas on civil rights until fairly recently.
  
  Einstein’s approach to problems in physics was to begin by asking very simple, almost childlike questions, such as, “What would the world look like if I could drive along a beam of light?” Gates said.
  
  “He must have developed his ideas about race through a similar process. He was capable of asking the question, ‘What would my life be like if I were black?’”
  
  Gates said that thinking about Einstein’s involvement with civil rights has prompted him to speculate on the value of affirmative action and the goal of diversity it seeks to bring about. There are many instances in which the presence of strength and resilience in a system can be attributed to diversity.
  
  “In the natural world, for example, when a population is under the influence of a stressful environment, diversity ensures its survival,” Gates said.
  
  On a cultural level, the global influence of American popular music might be attributed to the fact that it is an amalgam of musical traditions from Europe and Africa.
  
  These examples have led him to conclude that “diversity actually matters, independent of the moral argument.” Gates said he believes “there is a science of diversity out there waiting for scholars to discover it.”

Albert Einstein, Civil Rights Activist

Here’s something you probably don’t know about Albert Einstein.

Image:Einstein with the children of Lincoln University Faculty, May 3, 1946

In 1946, the Nobel Prize-winning physicist traveled to Lincoln University in Pennsylvania, the alma mater of Langston Hughes and Thurgood Marshall and the first school in America to grant college degrees to blacks. At Lincoln, Einstein gave a speech in which he called racism “a disease of white people,” and added, “I do not intend to be quiet about it.” He also received an honorary degree and gave a lecture on relativity to Lincoln students.

The reason Einstein’s visit to Lincoln is not better known is that it was virtually ignored by the mainstream press, which regularly covered Einstein’s speeches and activities. (Only the black press gave extensive coverage to the event.) Nor is there mention of the Lincoln visit in any of the major Einstein biographies or archives.

In fact, many significant details are missing from the numerous studies of Einstein’s life and work, most of them having to do with Einstein’s opposition to racism and his relationships with African Americans.

That these omissions need to be recognized and corrected is the contention of Fred Jerome and Rodger Taylor, authors of “Einstein on Race and Racism” (Rutgers University Press, 2006). Jerome and Taylor spoke April 3 at an event sponsored by the W.E.B. Du Bois Institute for African and African American Research. The event also featured remarks by Sylvester James Gates Jr., the John S. Toll Professor of Physics, University of Maryland.

According to Jerome and Taylor, Einstein’s statements at Lincoln were by no means an isolated case. Einstein, who was Jewish, was sensitized to racism by the years of Nazi-inspired threats and harassment he suffered during his tenure at the University of Berlin. Einstein was in the United States when the Nazis came to power in 1933, and, fearful that a return to Germany would place him in mortal danger, he decided to stay, accepting a position at the recently founded Institute for Advanced Study in Princeton, N.J. He became an American citizen in 1940.

But while Einstein may have been grateful to have found a safe haven, his gratitude did not prevent him from criticizing the ethical shortcomings of his new home.

“Einstein realized that African Americans in Princeton were treated like Jews in Germany,” said Taylor. “The town was strictly segregated. There was no high school that blacks could go to until the 1940s.”

Einstein’s response to the racism and segregation he found in Princeton (Paul Robeson, who was born in Princeton, called it “the northernmost town in the South”) was to cultivate relationships in the town’s African-American community. Jerome and Taylor interviewed members of that community who still remember the white-haired, disheveled figure of Einstein strolling through their streets, stopping to chat with the inhabitants, and handing out candy to local children.

One woman remembered that Einstein paid the college tuition of a young man from the community. Another said that he invited Marian Anderson to stay at his home when the singer was refused a room at the Nassau Inn.

Einstein met Paul Robeson when the famous singer and actor came to perform at Princeton’s McCarter Theatre in 1935. The two found they had much in common. Both were concerned about the rise of fascism, and both gave their support to efforts to defend the democratically elected government of Spain against the fascist forces of Francisco Franco. Einstein and Robeson also worked together on the American Crusade to End Lynching, in response to an upsurge in racial murders as black soldiers returned home in the aftermath of World War II.

The 20-year friendship between Einstein and Robeson is another story that has not been told, Jerome said, but that omission may soon be rectified. A movie is in the works about the relationship, with Danny Glover slated to play Robeson and Ben Kingsley as Einstein.

Einstein continued to support progressive causes through the 1950s, when the pressure of anti-Communist witch hunts made it dangerous to do so. Another example of Einstein using his prestige to help a prominent African American occurred in 1951, when the 83-year-old W.E.B. Du Bois, a founder of the NAACP, was indicted by the federal government for failing to register as a “foreign agent” as a consequence of circulating the pro-Soviet Stockholm Peace Petition. Einstein offered to appear as a character witness for Du Bois, which convinced the judge to drop the case.

Gates, an African-American physicist who has appeared on the PBS show Nova, said that Einstein had been a hero of his since he learned about the theory of relativity as a teenager, but that he was unaware of Einstein’s ideas on civil rights until fairly recently.

Einstein’s approach to problems in physics was to begin by asking very simple, almost childlike questions, such as, “What would the world look like if I could drive along a beam of light?” Gates said.

“He must have developed his ideas about race through a similar process. He was capable of asking the question, ‘What would my life be like if I were black?’”

Gates said that thinking about Einstein’s involvement with civil rights has prompted him to speculate on the value of affirmative action and the goal of diversity it seeks to bring about. There are many instances in which the presence of strength and resilience in a system can be attributed to diversity.

“In the natural world, for example, when a population is under the influence of a stressful environment, diversity ensures its survival,” Gates said.

On a cultural level, the global influence of American popular music might be attributed to the fact that it is an amalgam of musical traditions from Europe and Africa.

These examples have led him to conclude that “diversity actually matters, independent of the moral argument.” Gates said he believes “there is a science of diversity out there waiting for scholars to discover it.”

When Supermassive Supergiants Go Superboom

Article by Phil Plait via Slate

I have long been fascinated by gamma-ray bursts (or GRBs). These are incredibly violent events: It’s like taking the Sun’s entire lifetime energy output and cramming into a single event that lasts for mere seconds! The energy emitted is so intense, so bright, we can see GRBs from a distance of billions of light years.

Gamma rays themselves are just a form of light, like the kind we see, but with huge energy; each photon is packed with millions or billions of times the energy in a single photon of visible light. Only the most energetic events in the Universe can make them, so if we detect a burst of them coming from the sky, we know something literally disastrous has happened.

We know GRBs come in many flavors. Some last literally for milliseconds, while others stretch on for minutes. We also know different events can cause them, too. Short ones seem to come from merging neutron stars, ultra dense compact objects left over after stars explode. The longer ones occur when massive stars explode, leaving their cores to collapse. In both cases, the huge blast of high-energy gamma rays signals the birth of a black hole.

But astronomers were recently surprised to find a third type of GRB, one that lasts not for minutes, but for hours. Whatever these objects are, they don’t just flash with light, they linger, blasting out far, far more gamma rays for far, far longer than was previously thought. What could do such a thing?

Several ideas were put forth, but new observations provided the linchpin: an ultra-long-duration GRB occurred on Christmas Day in 2010, and its distance was found to be a soul-crushing 7 billion light years away, about halfway across the visible Universe! This left only one possible candidate for the progenitor: a hugely massive star, one so big it dwarfs the Sun into insignificance.

Continue to Full Article..


  Airglow, Gegenschein, and Milky Way
  
  As far as the eye could see, it was a dark night at Las Campanas Observatory in the southern Atacama desert of Chile. But near local midnight on April 11, this mosaic of 3 minute long exposures revealed a green, unusually intense, atmospheric airglow stretching over thin clouds.
  
  Image Credit & Copyright: Yuri Beletsky (Las Campanas Observatory, Carnegie Institution)
  
  Unlike aurorae powered by collisions with energetic charged particles and seen at high latitudes, the airglow is due to chemiluminescence, the production of light in a chemical reaction, and found around the globe. The chemical energy is provided by the Sun’s extreme ultraviolet radiation. Like aurorae, the greenish hue of this airglow does originate at altitudes of 100 kilometers or so dominated by emission from excited oxygen atoms.
  
  The gegenschein, sunlight reflected by dust along the solar system’s ecliptic plane was still visible on that night, a faint bluish cloud just right of picture center. At the far right, the Milky Way seems to rise from the mountain top perch of the Magellan telescopes. Left are the OGLE project and du Pont telescope domes.

Airglow, Gegenschein, and Milky Way

As far as the eye could see, it was a dark night at Las Campanas Observatory in the southern Atacama desert of Chile. But near local midnight on April 11, this mosaic of 3 minute long exposures revealed a green, unusually intense, atmospheric airglow stretching over thin clouds.

Image Credit & Copyright: Yuri Beletsky (Las Campanas Observatory, Carnegie Institution)

Unlike aurorae powered by collisions with energetic charged particles and seen at high latitudes, the airglow is due to chemiluminescence, the production of light in a chemical reaction, and found around the globe. The chemical energy is provided by the Sun’s extreme ultraviolet radiation. Like aurorae, the greenish hue of this airglow does originate at altitudes of 100 kilometers or so dominated by emission from excited oxygen atoms.

The gegenschein, sunlight reflected by dust along the solar system’s ecliptic plane was still visible on that night, a faint bluish cloud just right of picture center. At the far right, the Milky Way seems to rise from the mountain top perch of the Magellan telescopes. Left are the OGLE project and du Pont telescope domes.


  How do rockets move in space?
  
  If space is basically a vacuum and void of atmosphere, how do rockets alter the direction and speed of space craft? In other words, how do they “push off” against nothing?
  
  This is a very good question. Isaac Newton worked out the solution and published it in 1687 in his Principia Mathematica. It is phrased as Newton’s 3rd law. I’ll include all 3 below just in case!
  
  1st: A body will remain at rest or at motion with a uniform speed unless it is acted on my an external force.
  2nd: The acceleration of a body with a force acting on it is that force divided by the mass of the body (F=ma)
  3rd: Every action has an equal and opposite reaction.
  
  So the third law basically says that if you shoot out stuff in one direction you will move in the other direction. This is how rockets work in a vacuum. They have a source of fuel which is heated up so that it expands and is pushed out of the rocket. In order to change direction in space rockets have to have little ‘thrusters’ on all sides (you need 6 in total to maneuver completely in 3 dimensions).
  
  Newton’s 3rd law seems contrary to our intuition because on Earth there are lots of sources of friction - providing much easier methods of propulsion, however you might have seen it in action if you have ever blown up a balloon and then let go of it before tying it up. What pushes the balloon all around the room is the air you blew into in escaping.

How do rockets move in space?

If space is basically a vacuum and void of atmosphere, how do rockets alter the direction and speed of space craft? In other words, how do they “push off” against nothing?

This is a very good question. Isaac Newton worked out the solution and published it in 1687 in his Principia Mathematica. It is phrased as Newton’s 3rd law. I’ll include all 3 below just in case!

1st: A body will remain at rest or at motion with a uniform speed unless it is acted on my an external force. 2nd: The acceleration of a body with a force acting on it is that force divided by the mass of the body (F=ma) 3rd: Every action has an equal and opposite reaction.

So the third law basically says that if you shoot out stuff in one direction you will move in the other direction. This is how rockets work in a vacuum. They have a source of fuel which is heated up so that it expands and is pushed out of the rocket. In order to change direction in space rockets have to have little ‘thrusters’ on all sides (you need 6 in total to maneuver completely in 3 dimensions).

Newton’s 3rd law seems contrary to our intuition because on Earth there are lots of sources of friction - providing much easier methods of propulsion, however you might have seen it in action if you have ever blown up a balloon and then let go of it before tying it up. What pushes the balloon all around the room is the air you blew into in escaping.


  Balancing Rocks in Central Oregon
  
  “Geologists explain that the formations are the result of the aging, tilting and erosion of two layers of consolidated volcanic ash, known as tuff.
  
  These ash flows originated from the Cascade volcanoes to the west many thousands of years ago. The top layer of tuff was tougher so to speak than the bottom layer, so as the ground tilted and cracked and the softer bottom layer was eroded by wind and water, top-heavy rock pedestals remained.
  
  Discovered by surveyors way back in the 1850s, the unusual rocks were known to only a handful of people for many decades. They remained hidden in a forest of pine and juniper until a forest fire in 2002 denuded the area. Visible now from Forest Service roads and from boats on the popular Lake Billy Chinook below, the rocks are visited more frequently. Sadly, the formations pose an irresistible temptation to immature vandals and a few of the pedestals have been toppled. Fortunately, most are far more massive, stable and durable than they appear.”— Brad Goldpaint

Balancing Rocks in Central Oregon

“Geologists explain that the formations are the result of the aging, tilting and erosion of two layers of consolidated volcanic ash, known as tuff.

These ash flows originated from the Cascade volcanoes to the west many thousands of years ago. The top layer of tuff was tougher so to speak than the bottom layer, so as the ground tilted and cracked and the softer bottom layer was eroded by wind and water, top-heavy rock pedestals remained.

Discovered by surveyors way back in the 1850s, the unusual rocks were known to only a handful of people for many decades. They remained hidden in a forest of pine and juniper until a forest fire in 2002 denuded the area. Visible now from Forest Service roads and from boats on the popular Lake Billy Chinook below, the rocks are visited more frequently. Sadly, the formations pose an irresistible temptation to immature vandals and a few of the pedestals have been toppled. Fortunately, most are far more massive, stable and durable than they appear.”Brad Goldpaint

Neil deGrasse Tyson Connects with Rapper The GZA


  Have you seen the episode of StarTalk on the Nerdist Channel where Neil interviews GZA from the Wu-Tang Clan? If not, you can watch it below.
  
  In case you didn’t know it, Neil is not a Hip Hop fan. No, Neil is into the Blues, in a big way. And so he didn’t know much about GZA going into the interview. I watched as our producer and a Hip Hop aficionado (who also happened to be a postdoctoral researcher in physics at MIT) briefed Neil on “The Genius.”
  
  Then GZA came in to the studio, and I watched him and Neil get to know each other. On paper, the two don’t appear to have much in common, and at the start of the afternoon, it wasn’t certain that they’d end up that way, either.
  
  But then they got into the studio and the interview began. Slowly, GZA got comfortable with Neil, and they started to connect. And it turns out that they both have one very powerful thing in common: the universe is their muse.
  
  Listening to two people who have influence over others – who inspire those they touch to learn, to explore, to question – who are so very different in some ways, watching them come to understand and respect each other was a powerful experience, and I think it comes across in the video. I know everyone in the studio felt it that day.
  
  At one point Neil asks GZA how science factors into his creativity and what scientific idea is most intriguing. And GZA answers, “How everything is connected.”
  
  Clearly, one of the things that connects Neil and GZA is their love and awe for science. But there is something else that connects them, something that GZA puts best in the interview:
  
  “That’s one of the unique things about being an artist. That you have a voice that people hear and listen to, so it’s important to say something that’s important.”


Interview Can Be Found Here

Neil deGrasse Tyson Connects with Rapper The GZA

Have you seen the episode of StarTalk on the Nerdist Channel where Neil interviews GZA from the Wu-Tang Clan? If not, you can watch it below.

In case you didn’t know it, Neil is not a Hip Hop fan. No, Neil is into the Blues, in a big way. And so he didn’t know much about GZA going into the interview. I watched as our producer and a Hip Hop aficionado (who also happened to be a postdoctoral researcher in physics at MIT) briefed Neil on “The Genius.”

Then GZA came in to the studio, and I watched him and Neil get to know each other. On paper, the two don’t appear to have much in common, and at the start of the afternoon, it wasn’t certain that they’d end up that way, either.

But then they got into the studio and the interview began. Slowly, GZA got comfortable with Neil, and they started to connect. And it turns out that they both have one very powerful thing in common: the universe is their muse.

Listening to two people who have influence over others – who inspire those they touch to learn, to explore, to question – who are so very different in some ways, watching them come to understand and respect each other was a powerful experience, and I think it comes across in the video. I know everyone in the studio felt it that day.

At one point Neil asks GZA how science factors into his creativity and what scientific idea is most intriguing. And GZA answers, “How everything is connected.”

Clearly, one of the things that connects Neil and GZA is their love and awe for science. But there is something else that connects them, something that GZA puts best in the interview:

“That’s one of the unique things about being an artist. That you have a voice that people hear and listen to, so it’s important to say something that’s important.”

Interview Can Be Found Here