What is the Stratospheric
Observatory for Infrared Astronomy, or SOFIA, up to?
Stratospheric Observatory for Infrared Astronomy, as our flying telescope is called, is a Boeing 747SP aircraft
that carries a 2.5-meter telescope to altitudes as high as 45,000 feet.
Researchers use SOFIA to study the solar system and beyond using infrared
light. This type of light does not reach the ground, but does reach the
altitudes where SOFIA flies.
Recently, we used SOFIA to study water on Venus, hoping to
learn more about how
that planet lost its oceans. Our researchers used a powerful instrument on
SOFIA, called a spectrograph,
to detect water in its normal form and “heavy water,” which has an extra
neutron. The heavy water takes longer to evaporate and builds up over time. By
measuring how much heavy water is on Venus’ surface now, our team will be able
to estimate how much water Venus had when the planet formed.
We are also using SOFIA to create a detailed map of the Whirlpool
Galaxy by making multiple observations of the galaxy. This map will help us
understand how stars form from clouds in that galaxy. In particular, it will
help us to know if the spiral arms in the galaxy trigger clouds to collapse
into stars, or if the arms just show up where stars have already formed.
We can also use SOFIA to study methane on Mars. The Curiosity rover
has detected methane
on the surface of Mars. But the total amount of methane on Mars is unknown and
evidence so far indicates that its levels change significantly over time and
location. We are using SOFIA to search for evidence of this gas by mapping the Red
Planet with an instrument specially tuned to sniff out methane.
Next our team will use SOFIA to study Jupiter’s icy moon Europa, searching for evidence of possible water plumes detected by the Hubble Space Telescope. The plumes, illustrated in the artist’s concept above, were previously seen in images as extensions from the edge of the moon. Using SOFIA, we will search for water and determine if the plumes are eruptions of water from the surface. If the plumes are coming from the surface, they may be erupting through cracks in the ice that covers Europa’s oceans. Members of our SOFIA team recently discussed studying Europa on the NASA in Silicon Valley Podcast.
This is the view of Jupiter and its moons taken with SOFIA’s
light guide camera that is used to position the telescope.
Filters are very important in astronomical observation as they reduce glare and light scattering, increase contrast through
selective filtration, increase definition and resolution, reduce
irradiation and lessen eye fatigue.
Working of a magenta filter
Depending on which object you are looking, one chooses the appropriate filter. For instance the cover photo is without and withthe moon filter.
And on an amateur telescope they is how they are inserted.
The Crab Pulsar (PSR B0531+21) is a relatively young neutron star. The
star is the central star in the Crab Nebula, a remnant of the supernova
SN 1054, which was widely observed on Earth in the year 1054.Discovered
in 1968, the pulsar was the first to be connected with a supernova
The optical pulsar is roughly 20 km in diameter and the pulsar
“beams” rotate once every 33 milliseconds, or 30 times each second
The above video allows you to hear the signal from pulsar and the gif below that is the actual pulsar blinking taken with a high speed technique known as Lucky Imaging .
Robert Evans is the world record holder for the most visual discoveries of Supernovae. Although he is a minister of the uniting church in Australia, he is better known in the Astronomy community as one of the ‘best Amateur Astronomers in the world.’
He is accredited for discovering 42 supernovas visually from his backyard!!
But, how on earth does he do it ?
Having been looking at the cosmos for years on end, Evans has memorized the entire star field and the positions of the galaxies in the night sky.
And as a result of this, he can detect changes in the galaxy simply by looking at them through the telescope.
Why is this remarkable ?
This is truly remarkable for two pivotal reasons:
A supernova is the explosion of a star. It is the largest explosion that takes place in space.
But spotting a supernova visually is extremely hard!
To give a perspective on the intricacies of supernova hunting, here is a picture showing the night sky before and after a supernova in Messier-82.
Supernova hunting in Messier-82
And secondly, he gave automated telescopes a run for their money. There are many telescope in recent times that automatically detect hundreds of supernovas every year.
But Evans managed to give them a tough fight in a battle against man and technology with his telescope sorcery.
A note for budding astronomers
Why I find Evans to be extremely inspiring is because here is an amateur astronomer doing quality contributions to Astronomy in his backyard and with not so fancy equipment.
Just shows how far passion and perseverance can take you in science.
Haha.. I really appreciate the fact that you were curious about the moon’s photograph that is featured on a late night talk show.
Conan the talk show premiered on November 8, 2010. But it was a waxing crescent on November 8,2010 at 11:00 pm, Los Angeles CA.
And if one were to be really nitpicky about this,by 6:30pm on November 8, 2010 the moon would have already set and you most certainly would not see the moon on the night sky at 11pm.
Therefore, not really sure what the moon is trying to represent here.
Also the moon keeps changing its orientation over the course of one day. And if you decided to look at the moon each day at the same time , it would be look slightly different.
Moon over the course of 24 hours
But the moon on Conan’s show is mostly Static.
Unless he decides to replace the already ridiculously big moon (Diameter: 3,475 km) that only is supposed to occupy ~0.00106% of the celestial hemisphere in the night sky by a Death Star (Diameter: 100 km to 160km ) of the same size!
So.. I guess that answers your question.. Have a good one!