All of the Above

  • Random
  • Archive
  • RSS
  • Ask me anything
'\x3ciframe width=\x22500\x22 height=\x22281\x22 src=\x22http://www.youtube.com/embed/yDNAk0bwLrU?wmode=transparent\x26autohide=1\x26egm=0\x26hd=1\x26iv_load_policy=3\x26modestbranding=1\x26rel=0\x26showinfo=0\x26showsearch=0\x22 frameborder=\x220\x22 allowfullscreen\x3e\x3c/iframe\x3e'

laboratoryequipment:

Telescopes Help Study Atmospheres of Far-Off Worlds

Gone are the days of being able to count the number of known planets on your fingers. Today, there are more than 800 confirmed exoplanets – planets that orbit stars beyond our sun – and more than 2,700 other candidates. What are these exotic planets made of? Unfortunately, you cannot stack them in a jar like marbles and take a closer look. Instead, researchers are coming up with advanced techniques for probing the planets’ makeup.

One breakthrough to come in recent years is direct imaging of exoplanets. Ground-based telescopes have begun taking infrared pictures of the planets posing near their stars in family portraits. But to astronomers, a picture is worth even more than a thousand words if its light can be broken apart into a rainbow of different wavelengths.

Read more: http://www.laboratoryequipment.com/videos/2013/05/telescopes-help-study-atmospheres-far-worlds

I found this gem on my dashboard. This is in part the work of the space telescope high contrast group (the group I work in). AMNH always makes such nice movies! 

    • #exoplanets!
    • #atmospheres on other worlds!
    • #All the exclamations!
  • 4 days ago > laboratoryequipment
  • 9
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

The Baltimore Charter for Women in Science

Compared to most of the physical sciences women have much better representation in astronomy. My own personal experience here in Baltimore has been observing an extremely welcoming and comfortable atmosphere at the Space Telescope Science Institute. There are many women at the institute, it is family friendly, they offered same-sex couple benefits before Maryland passed marriage equality, etc. It seems that most people are respectful of each other, regardless of their official position (at least that is the vibe of the culture). I don’t usually think twice about how this kind of atmosphere developed, but it’s definitely something I really enjoy about working here. 

So it’s nice to learn a little about the history of the Institute and astronomy in general. Which brings me to the Baltimore Charter. The Baltimore Charter was a statement written in 1992 to address the attitude toward women in astronomy. This charter is an acknowledgment  of diversity’s benefit to science and a flawed culture in astronomy that does not encourage it. It suggests the steps to transform the culture and it has been a real turning point for the field as a whole, especially in Baltimore. To read about the 1992 “Meeting on the Status of Women in Astronomy” go here.

I’ll share one short excerpt from the charter:

“Our focus is on women but actions taken to improve the situation of women in astronomy should be applied aggressively to those minorities even more disenfranchised.”

If there ever was strong evidence that these biases need to be acknowledged and addressed, the charter is it. Astronomy in Baltimore has been a huge success story for women. And while we’ve come a long way, there is still work to do. There are more underrepresented groups who are discouraged in STEM fields and the conversation continues.

An illustration from the conference. How much can we say this picture has changed today?

Let’s keep the conversation going. Our job is not over. Feel free to leave any thoughts.

    • #BaltimoreCharter
    • #Astronomy
    • #WomenInScience
    • #DiversityIsBetterForScience
  • 1 month ago
  • 2
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

A Day To Remember

Today is Holocaust Remembrance Day, or Yom HaShoah. I made some comments on this day last year. The sentiment remains the same. Today is the day to remember how precious human life is, to remember what it means to be human, to have compassion, to move one step father from the bias and cruelty of past generations, one step closer to a world-wide community. 

Today is not only to remember the tragedies and traumas of our own families, but of all those who suffered at the hands of ruthlessness, ugliness, and neglect and those who still suffer today. We are all survivors. 

The slogan today is often “remember six million.” But let’s remember the more than six million, not only our own families, who perished when people stopped being people and turned their eyes away. Let’s make a commitment to integrity and empathy in our daily lives. 

Let us celebrate the best parts of humanity and confront the very worst. It is only through our consciousness and cooperation that we transform ourselves from a coincidental assembly of molecules drifting through space into a collective something that is aware of its own importance. However you celebrate, celebrate today. Celebrate in every moment that you remember what it means to be human. No one is exempt and no one is excluded.  

  • 1 month ago
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

The Ignition Grant!

Last Thursday night a few representative of our physics grad outreach attended Ignite Baltimore, a series of 5-minute, 20-slide talks about interesting/exciting/thoughtful ideas. It was a lot of fun and intriguing for sure — I’ll definitely go back. Another great thing about this group is that they award 2 grants each session for project that will make Baltimore a better place.

This year we submitted an application for this grant to sponsor a portable planetarium project, and last Thursday night we were awarded the grant! You guys, this is really happening. We are officially funded to do something. 

So what are we doing anyway?

We plan to use the free software from WWT and their network of software “ambassadors” to train a whole bunch of us in using the software as a teaching tool. We will also follow an off-the-shelf DIY planetarium construction plan to build a portable planetarium. The software interfaces with a projector and all that’s left is buying a spherical mirror to project the sky onto our planetarium. 

You can see an example here at WWT’s do-it-yourself dome project site.

We will build one as a prototype for us to keep and travel around with for astronomy workshops. We will also build a second planetarium at The Southwest Baltimore Charter School, with the students. They will get to keep this one. We’ll train the teachers and encourage the students to use the resource for class projects, etc. 

Anyone in the Baltimore area who is interested in getting involved in this should totally do it! Feel free to check out our new facebook page: http://www.facebook.com/PAGSOutreach which should start to have more updated information on our activities. 

    • #IB12
    • #ignitebaltimore
    • #WWT
    • #astronomy is for everyone
    • #bringing the skies to baltimore
  • 1 month ago
  • 2
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

Stand Up For STEM Outreach and Education

For me, a big part of my experience in grad school is the outreach that many of my colleagues have joined together to deliver to the community. We all understand the importance of better STEM (Science, Technology, Engineering, & Mathematics) education and how its current state is less than spectacular across the country. I think that most all forms of outreach/charity/volunteer involvement with the intent of inclusion and enriching the local and global community are valuable efforts towards a better world. STEM is my passion and the way that I wish to contribute to the overall effort. 

So it is not a surprise that myself and many of my friends and colleagues are shocked by NASA’s recent suspension of public outreach. Not only is the outreach directed toward inspiring future generations of scientists and engineers, it is also the public face of NASA, which means a long-term strategy for funding. Sure, when we think of the great achievements of NASA we point to the science and missions, but public exposure and carefully & creatively constructed explanations of these activities would not be possible without NASA’s public relations. 

But let’s be a little clearer about what we’re missing out on. It’s not only what we normally consider “education and outreach” projects that have been suspended. According to the memo suspended activities include:

- Programs, events, and workshops. 

- Permanent and traveling exhibits, signage, and other materials. 

- Speeches, presentations, and appearances, with the exception of technical presentations by researchers at scientific and technical symposia. 

- Video and multimedia products in development (and renewal of existing products). 

- Web and social media sites in development (excludes operational sites). 

- External and internal publications, with the exception of Scientific and Technical Information as defined by NPD 2200.1B. 

- Any other activity whose goal is to reach out to external and internal stakeholders and the public concerning NASA, its programs, and activities.

By the way, “programs, events, and workshops” include both educational and scientific ones. And this last broad point about “any activity” that reached out to stakeholders and the public makes me pretty uncomfortable. Could these short term cuts limit or discontinue NASA’s support and collaboration with private agencies (like SpaceX for example) and external contractors? This is not just about halting NASA facebook updates; the impacts are a pretty big deal and if this goes on too long it will come to affect many of us in astronomy and the greater STEM community. 

I don’t know how much signing this petition will help, but getting the government to pay attention is not a bad idea. 

I also recommend writing to the White House and other representatives about this issue and the sequester in general. I certainly will. 

I’m not trying to bash NASA here, more the lack of interest in pursuing and supporting STEM education. NASA is in an unfortunate position right now and we can hopefully help by putting some pressure on our representatives. 

  • 1 month ago
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

Adventures in Equador - Part 2: Pressure!

On this trip we were staying mostly in the city of Quito, the capitol. Quito is at about 9k feet above sea-level. The city is carved into a chain of mountains, so there’s quite a bit of elevation change between the lowest and tallest points. 

image

Having a few scientists on the trip inspired some of the usual nerdy activity. During one evening we took cable cars up to about 13k feet, where we were literally above the clouds!

image

We took an open water bottle up on our ascent and closed it shut at the top (that is as after we got over the breathtaking view at sunset). Atmospheric pressure is lower at elevation, meaning the atmosphere is more diffuse. By closing the bottle we captured this pressure for our own quick experiment. We kept it closed all the way back to sea-level after the trip ended, and this is what happened:

image

Pressure is a force over an area. Back at sea-level where pressure is higher, there is more force pushing inward on the outside of the bottle than there is pushing outward from inside the bottle, so it gets crushed! Ecuadorians must make their Guitig bottles well, because it is still sitting in this same condition in my office. 

  • 2 months ago
  • 1
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

Adventures in Ecuador, Part 1-Revisiting the Coriolis Effect

I spent the end of the winter holiday and new years in Ecuador this year. It was a huge ton of fun and I certainly learned a lot. I got the chance to visit the site of the equator, which brings up some interesting physics… as well as some entertaining pseudo-science.

image

Talking about the northern and southern hemispheres always brings up the “Coriolis effect.” The Coriolis force is not a real force at all, just a consequence of living on a rotating body (Earth). The way we see this effect on earth is in storm systems that are oriented counterclockwise in one hemisphere and clockwise in the other. 

image

Take it from this weather expert who uses real phenomena to describe what is happening rather than describing fictitious forces (http://weatherquesting.com/hurricane-spin.htm):

Why does the air spin?  The air masses that make up a hurricane move towards the low-pressure area, pushed by surrounding higher- pressure air.  But, because Earth’s surface spins at different speeds (faster at the equator, slower near the poles), air doesn’t move in a straight line from high to low pressure. 

The best example of the Coriolis force is on a merry-go-round. When trying to toss a ball to your buddy on a spinning merry-go-round, the ball seems to curve instead of going straight. You could call this a force (Coriolis force) pushing the ball, or you could observe the toss from outside the spinning merry-go-round and see that the ball goes straight; The merry-go-round is moving. Likewise, our earth is moving, so anything moving along some slice of the earth will appear to curve. I saw a nice video made by some grad students from U. of Illinois here.

For water flowing down a sink/bath tub drain, however the difference in the speed of the earth between the top and bottom of this spinning vortex is minuscule. Just think about the size of the Earth compared to the size of a tiny sink vortex. This brings me to some demonstrations I saw at the equator. Our guide “demonstrated” the Coriolis effect by draining a tub north of, south of, and on the equator. Naturally, to our delight, water did not spin down the drain on their line for the equator, clockwise north of the equator, and counterclockwise on the south side. A real crowd pleaser!

image

You can see: “at the equator,” “north of the equator,” and “south of the equator.”

Now I had quite a bit of egg on my face after telling everyone days before that water did not flow differently down drains in the different hemispheres. And since this incident I’ve done very rough calculations for my own sanity check that lead to deflects on the order of microns or smaller (think shorter than the width of a human hair). It can be easy to force the water in one direction or another without much effort (it’s a small enough effect). But the middle step of draining the tub without any spinning really stumped me. I can only conclude that I don’t know enough about the container she used. Maybe there was some sleight of hand?

I know it seemed like a controlled demonstration, but we didn’t see it more than once. While it sounds like a cop-out, an experiment has to be repeatable. If published in a scientific journal this would be held under incredible scrutiny, requiring the elimination of all other sources of rotation. If only we could verify the necessary conditions for observing (or not observing) the Coriolis effect in a draining tub. Lucky for us, scientists are curious people. One Ascher Shapiro conducted this experiment at MIT in 1962. After eliminating any other motions, it took 12-15 minutes to see the effects of the Coriolis “force.” You can read about it here in an MIT tech review. Yes you can observe the Coriolis effect in a draining tub, but it is a tiny tiny tiny effect.

If you’re wondering how the guides at the equator accomplished the trick, there are people out there on the internet who have some hunches, like here, where you can find instructions for reproducing this trick under “do-it-yourself fakery”

And on that note, llamas:

image

  • 3 months ago
  • 2
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

The Awesomest

Had to share from some photos I recently took. A James Webb Space Telescope interactive display to help get a sense of just how immense the JWST mirror is. 

image

The picture doesn’t exactly do it justice, but it was pretty darn impressive. JWST is the next big thing in space-based astronomy. When I say big I don’t just mean the budget (though that is certainly non-trivial), but the biggest space-telescope mirror. JWST will follow up Hubble’s legacy of startlingly beautiful images of objects ranging from local star clusters to the very first galaxies, all the way to the beginnings of the universe. But even better than stunning images will be the amazing science - technologies aboard that will push countless boundaries of space-based observing. 

JWST will succeed Hubble in a few key ways. For one, the size. The bigger the telescope, the better the resolution possible. Here’s a really good figure showing the relative scale from the fine folks at NASA:

image

It’s really hard to send a large mirror up into space so most space telescopes have a pretty modest size. JWST achieves this jump in effective diameter because its mirror is in segments. The whole thing is folded up and opens once it reaches the destination. While JWST is around 6.5 m, the largest ground telescopes are 8-10, and we’ve got our sights on 30 m or more down the line. 

While Hubble is in orbit around the Earth, JWST will orbit around a stable point in the Earth-Sun system. Hubble can only observe part of the time (when it isn’t in the sun). Meanwhile, JWST will always point away from the sun and be able to observe more continuously. How far away from Earth is it? About a tenth the distance between the Earth and the Sun (in the opposite direction). The image below shows the various “stable” points in the Sun-Earth system. It is not to scale. L2 will always remain in this location relative to the sun and the Earth. 

image

One last key improvement on Hubble is how cool the telescope will be. In order to observe infrared radiation, the instruments have to be extremely cold. JWST is equipped with a massive sun shield and a sophisticated cooling system. Seeing in the infrared allows us to see cooler and farther than we’ve seen before with a space telescope.

It really is the awesomest.

image

    • #JWST
    • #The Awesomest
    • #Space Telescope
    • #One Excited Astronomer
  • 3 months ago
  • 2
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+

Laboratory Equipment: IBM’s Watson is Off to College

laboratoryequipment:

Watson, the supercomputer famous for beating the world’s best human “Jeopardy!” champions, is going to college.

IBM is announcing today that it will provide a Watson system to Rensselaer Polytechnic Institute, in New York state, the first time the computer is being sent to a university. Just like…

My alma mater! Looks like RPI is attracting some unconventional students…

  • 3 months ago > laboratoryequipment
  • 17
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+
rabraha3:

Nowadays we see images like this, bright lasers shining from the worlds largest optical telescopes. Why do we need lasers? It is for a system called adaptive optics.
Normally, the atmosphere limits the resolution of a telescope on the ground. This is one reason why the biggest observatories are in dry regions at high altitudes. But we can now actively correct for the distortion due to the atmosphere!
Adaptive optics requires a deformable or segmented mirror.

Computers can control the alignment of each segment individually. Essentially what happens is the telescope looks at a star, which should be a point source, but the atmosphere has smeared it out. A computer moves each segment to take the smudge and make it into a point. This happens something like 60 times per second, so we need a really bright source — a source that emits enough light to be seen in 0.016 s.
That’s where the laser comes in. One can use a laser to excite sodium atoms ~20 km above sea level. The laser creates a bright spot of sodium emission, which can be used like a star to guide the computer. A .gif of adaptive optics in action from wiki:

On the left what what we’d normally see through this telescope, and on the right is the corrected image. Excellent! Some results:

And:

The binary star IW Tau, with a separation of 0.3 arcsec (8.3e-5o). Oh technology, how very clever. We don’t have to rely on space-based telescopes to get the best resolution anymore. So people are now talking about a 30m telescope at Hawaii and a 39m telescope, the European Extremely Large Telescope.


This is a great post, and certainly a topic very close to my heart. I do, however, want to make a case for space telescopes even with adaptive optics on the ground. First of all, while adaptive optics can significantly correct the wavefront, it isn’t perfect. The wavefront is much more stable in space and doesn’t rely on a quickly changing deformable mirror and a matching high-speed control system. This stability allows us to do imaging at diffraction-limited resolution and also maintain great contrast for high-contrast imaging techniques. The telescopes we put in space are all smaller than our biggest ground telescopes — and we still need them. 
Another reason we go to space is that the atmosphere doesn’t only change the shape of the wavefront, but it also absorbs light — light that will never reach the ground to be corrected an imaged. For one example, this is a problem in the mid-infrared where the molecules in the atmosphere absorb this kind of energy. For this range of energies (among others) it is still useful to go into space. 
The graphic below is taken from this website, credit: NASA/IPAC. 


So, I thank rabraha3 for explaining that we don’t need space telescopes for their resolution — we can certainly accomplish that from the ground with the help of adaptive optics. However, space telescopes have different systematics to correct for and there is definitely still a place for them.
The next stage of extremely large telescopes will have to have extremely sophisticated adaptive optics systems, beyond the capability of current technology. These present very exciting engineering challenges for the future. These new telescopes will give us HUGE improvements in resolution. I am certainly looking forward to the science we’ll be capable of.
For more about the Thirty Meter Telescope project: http://www.tmt.org/about-tmt
Pop-upView Separately

rabraha3:

Nowadays we see images like this, bright lasers shining from the worlds largest optical telescopes. Why do we need lasers? It is for a system called adaptive optics.

Normally, the atmosphere limits the resolution of a telescope on the ground. This is one reason why the biggest observatories are in dry regions at high altitudes. But we can now actively correct for the distortion due to the atmosphere!

Adaptive optics requires a deformable or segmented mirror.

image

Computers can control the alignment of each segment individually. Essentially what happens is the telescope looks at a star, which should be a point source, but the atmosphere has smeared it out. A computer moves each segment to take the smudge and make it into a point. This happens something like 60 times per second, so we need a really bright source — a source that emits enough light to be seen in 0.016 s.

That’s where the laser comes in. One can use a laser to excite sodium atoms ~20 km above sea level. The laser creates a bright spot of sodium emission, which can be used like a star to guide the computer. A .gif of adaptive optics in action from wiki:

image

On the left what what we’d normally see through this telescope, and on the right is the corrected image. Excellent! Some results:

image

And:

image

The binary star IW Tau, with a separation of 0.3 arcsec (8.3e-5o). Oh technology, how very clever. We don’t have to rely on space-based telescopes to get the best resolution anymore. So people are now talking about a 30m telescope at Hawaii and a 39m telescope, the European Extremely Large Telescope.

This is a great post, and certainly a topic very close to my heart. I do, however, want to make a case for space telescopes even with adaptive optics on the ground. First of all, while adaptive optics can significantly correct the wavefront, it isn’t perfect. The wavefront is much more stable in space and doesn’t rely on a quickly changing deformable mirror and a matching high-speed control system. This stability allows us to do imaging at diffraction-limited resolution and also maintain great contrast for high-contrast imaging techniques. The telescopes we put in space are all smaller than our biggest ground telescopes — and we still need them. 

Another reason we go to space is that the atmosphere doesn’t only change the shape of the wavefront, but it also absorbs light — light that will never reach the ground to be corrected an imaged. For one example, this is a problem in the mid-infrared where the molecules in the atmosphere absorb this kind of energy. For this range of energies (among others) it is still useful to go into space. 

The graphic below is taken from this website, credit: NASA/IPAC. 

Atmospheric Opacity

So, I thank rabraha3 for explaining that we don’t need space telescopes for their resolution — we can certainly accomplish that from the ground with the help of adaptive optics. However, space telescopes have different systematics to correct for and there is definitely still a place for them.

The next stage of extremely large telescopes will have to have extremely sophisticated adaptive optics systems, beyond the capability of current technology. These present very exciting engineering challenges for the future. These new telescopes will give us HUGE improvements in resolution. I am certainly looking forward to the science we’ll be capable of.

For more about the Thirty Meter Telescope project: http://www.tmt.org/about-tmt

  • 3 months ago > rabraha3
  • 19
  • Permalink
Share

Short URL

TwitterFacebookPinterestGoogle+
Page 1 of 5
← Newer • Older →

About

Avatar Alex Greenbaum
Astrophysicist, Female
  • About Me

Following

  • laboratoryequipment
  • mydrunkkitchen
  • fishingboatproceeds
  • edwardspoonhands
  • isitisabel
  • dresdencodak
  • alex-day-music
  • curtislaraque
  • beatonna
  • grumwave
  • staff
  • rabraha3
  • aidosaur
  • s4mpuff
  • marlomeekins
  • gunnerkrigg
  • thestephareno
  • lookslikescience
  • starlightgirl888
  • matthewvonhumboldt
  • chickinwings

Top

  • RSS
  • Random
  • Archive
  • Ask me anything
  • Mobile
Effector Theme by Pixel Union