Stars Are Cool. No, Really, They Are


When the gringa’s dear readers think of a star, what do you think of? The Sun? Polaris? Alpha Centauri?  And what do you think would happen if you reached out to touch the Sun? You’d probably get vaporized, right? Well, depending on the star, not necessarily. In fact, if you touched the right star it might be a sensation more like when you roll over in bed and find the cool spot.

Brown dwarfs are cold stars. There are 14 that NASA believes are cool enough to touch. Cool! They are also the oldest stars in the Universe. I guess stars are kind of like people. Old folks with poor circulation are generally cold all the time. Stars get old and cold, too. Out of all the old, cold, brown dwarf stars in the Universe, it’s the Y-dwarfs that are even cooler than the average human’s body temperature. Y, you may ask. Well, the gringa will tell you why the Y is the way that it is.

Not only are they old but they are failures. Poor Y-dwarfs. They must have very low self-esteem. Perhaps that is why they don’t shine as brightly as other stars. They have grown old and are failures as stars. The gringa feels very sorry for the poor, little things.

Because their cores are not very dense they can’t fuse loads of atoms within. That means they don’t burn as hot and brightly as other stars. The gringa finds it very amusing that the denser a star is the brighter it is. It doesn’t seem to work that way in humans.

If Y-dwarfs are such failures at being stars, the gringa wonders if they should be considered stars at all. Do we have a Pluto prospect in the future? Just as Pluto got demoted from planet to dwarf planet, Y-dwarf stars may very well face the possibility of being re-classified. In the future scientists may decide they don’t meet all the guidelines of being a star. The gringa thinks this is a wonderful possibility for Y-dwarfs. Whereas poor Pluto suffered a demotion, the Y-dwarf could get better news. They could go from being failures as stars to being over-achievers for whatever it is they may become!

However, it may take astronomers quite some time to collect enough data in their studies. Their failure to shine bright like a diamond in the sky means it is difficult to view and study them. It’s practically impossible to study them at all with a telescope dependent on visible light. To take productive peeks at Y-dwarfs NASA had to construct an infrared telescope and mount it to an orbiting satellite. And that is why the Universe is wiser thanks to these cold, little star failures, because of Wide-field Infrared Survey Explore (WISE) that studies them in the heavens.

Source:  www.nasa.gov

Image Credit:  www.jpl.nasa.gov

 

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Isaac Newton By The Sea


NASA recently reported images of an X-ray tail (or, ribbon) of galactic gas. It has broken cosmic records with the extraordinary length of 250,000 light years. The published images are a composite from combined data that originated from the Chandra orbiting observatory and the Isaac Newton Group (ING) of Telescopes that are located in the Canary Islands of Spain.

ING consists of two telescopes. One is named William Herschel (WMT) and the other is Isaac Newton (INT). They are located on a seaside cliff of La Palma Island and command a breathtaking view of the sea as well as the night sky. Isaac Newton began serving astronomers in 1984 and William Hershel in 1987.

ING is a collaborative effort of scientists representing the United Kingdom, the Netherlands and Spain. Their goals in serving the world community of astronomers and space related science is to provide world class telescope operations and programs that aid in research efforts. To encourage innovative methods in science and research, ING welcomes projects that involve novel instruments as “visitors”.  ING is committed to fostering original thinking as well as strongly supporting classical observing.

The Isaac Newton Telescope is open for visiting observers. New instruments are now being enjoyed with funding to provide more. One new instrument, the PAUCam, is a state of the art imaging device that creates prime focus capabilities for the William Hershel Telescope. A wide-field multi-object spectrograph is being developed for William Hershel and expected to become operational in 2017. This instrument will be part of a five year study to help understand how the Milky Way was “assembled”.

WEAVE is the name of the spectrograph developed for William Hershel. WEAVE was designed and built by a consortium of institutes from the UK, the Netherlands, Spain and France. Although visitors will still have access to observe the heavens through William Hershel, much of the telescope’s time will be devoted to the study of three particular projects: 1. The archaeology of the Milky Way; 2. The evolution of the galaxy; 3. Dark energy and its nature. These projects create wonderful opportunities for the UK, the Netherlands and Spain to make important scientific contributions to the world community’s knowledge of outer space.

Resident student programmes are available with ING. Over the past decade, forty students have served in the position of INT support astronomers and have gained valuable hands-on experience and technical skills. In fact, since 2009, 53 PhD theses have been based on ING data. Announcements will be made in March 2016 about the details of the 2016/2017 programme which offers astronomy and astrophysics PhD’s, MSc’s. INT welcomes students who are interested in any field of astronomy or astronomical instrumentation.

Students stay in flats provided by ING and receive a modest monthly stipend. These are cozy abodes within walking distance to the observatories, however, ING also provides transportation back and forth. For one year students will have the opportunity to participate in supportive roles in the work performed by one of the world’s most scientifically productive and versatile telescope groups. They will become part of the professional astronomical family of La Palma.

To qualify for admission to the programme, students must be a European citizen or European student resident. Enrollment in an astronomy PhD or MSc program or in the final year of undergraduate astronomy or physics course is required. English is a must, Spanish is a plus. It is also helpful to have some experience with Linux/UNIX operating systems as well as IRAF astronomical data reduction software. While participating in the program, expect to work 37 hours weekly, day or night, as well as weekends and holidays. A valid driving license is expected as well as being able to pass a medical examination.

Four positions are available. Students report for duty in September. During the one year of service, students have a 25 day leave allowance.

Qualified students who are interested should prepare a cover letter presenting experience along with any other pertinent information to be considered. Two references are required. Applications must be received by May 1 via e-mail or snail-mail. E-mail contact is Ovidiu Vaduvescu, INT studentship program manager, ovidiuv@ing.iac.es. Snail mail contact info:

Studentship Programme Manager

Isaac Newton Group of Telescopes

Apartado de coreos 321, E-38700, Santa Cruz de La Palma, SPAIN

Fax: +34 922 425 401

And, if you are unqualified, like the gringa, but still interested in what goes on at ING, their website has an interesting feature that the gringa really likes. It’s called “Ask an Astronomer!”. You simply fill out the e-mail form and submit. It’s not just any ol’ email form, however. It also has lots of other information to pick and choose from. Click “send” and wait for an amazing scientist to school you on what you want to know.

Source: www.ing.iac.es

Photo Credit: en.wikipedia.org