Uploaded June 2010 | Updated September 2026, 1 week ago
facebook.com/ScienceReason ... Look for dark interstellar clouds blocking patches of Milky Way stars! What's up for July 2010: Dark Nebulae in the Milky Way Galaxy ... with Jane Houston Jones at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California.
---
Please SUBSCRIBE to Science & Reason:
• youtube.com/Best0fScience
• youtube.com/ScienceTV
• youtube.com/FFreeThinker
• youtube.com/RationalHumanism
---
We live in the Milky Way Galaxy. If you were looking down on the Milky Way, it would look like a large pinwheel rotating in space. Our Galaxy is a spiral galaxy that formed approximately 14 billion years ago. Contained in the Milky Way are stars, clouds of dust and gas called nebulae, planets, and asteroids. Stars, dust, and gas fan out from the center of the Galaxy in long spiraling arms. The Milky Way is approximately 100,000 light-years in diameter. Our solar system is 26,000 light-years from the center of the Galaxy. All objects in the Galaxy revolve around the Galaxy's center. It takes 250 million years for our Sun (and the Earth with it) to make one revolution around the center of the Milky Way.
When you look up at the night sky, most of the stars you see are in one of the Milky Way arms. Before we had telescopes, people could not see many of the stars very clearly. They blurred together in a white streak across the sky. A myth by the ancient Greeks said this white streak was a "river of milk". The ancient Romans called it the Via Galactica, or "road made of milk". This is how our Galaxy became known as the Milky Way. It is interesting to note that astronomers capitalize the "G" in galaxy when talking about our Milky Way!
Today, astronomers have been able to observe the Milky Way in all regions of the electromagnetic spectrum. They have had to be clever in making the observations since they are having to look through the disk of the Galaxy from our location in one of the arms! Below, you can see that the Milky way looks very different in different wavelengths of light. You can read more about this at the Multiwavelength Milky Way Web site.
• imagine.gsfc.nasa.gov/docs/features/objects/milkyway1.html
• mwmw.gsfc.nasa.gov/mmw_edu.html
.
facebook.com/ScienceReason ... Look for dark interstellar clouds blocking patches of Milky Way stars! What's up for July 2010: Dark Nebulae in the Milky Way Galaxy ... with Jane Houston Jones at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California.
---
Please SUBSCRIBE to Science & Reason:
• youtube.com/Best0fScience
• youtube.com/ScienceTV
• youtube.com/FFreeThinker
• youtube.com/RationalHumanism
---
We live in the Milky Way Galaxy. If you were looking down on the Milky Way, it would look like a large pinwheel rotating in space. Our Galaxy is a spiral galaxy that formed approximately 14 billion years ago. Contained in the Milky Way are stars, clouds of dust and gas called nebulae, planets, and asteroids. Stars, dust, and gas fan out from the center of the Galaxy in long spiraling arms. The Milky Way is approximately 100,000 light-years in diameter. Our solar system is 26,000 light-years from the center of the Galaxy. All objects in the Galaxy revolve around the Galaxy's center. It takes 250 million years for our Sun (and the Earth with it) to make one revolution around the center of the Milky Way.
When you look up at the night sky, most of the stars you see are in one of the Milky Way arms. Before we had telescopes, people could not see many of the stars very clearly. They blurred together in a white streak across the sky. A myth by the ancient Greeks said this white streak was a "river of milk". The ancient Romans called it the Via Galactica, or "road made of milk". This is how our Galaxy became known as the Milky Way. It is interesting to note that astronomers capitalize the "G" in galaxy when talking about our Milky Way!
Today, astronomers have been able to observe the Milky Way in all regions of the electromagnetic spectrum. They have had to be clever in making the observations since they are having to look through the disk of the Galaxy from our location in one of the arms! Below, you can see that the Milky way looks very different in different wavelengths of light. You can read more about this at the Multiwavelength Milky Way Web site.
• imagine.gsfc.nasa.gov/docs/features/objects/milkyway1.html
• mwmw.gsfc.nasa.gov/mmw_edu.html
.
![NASA Astronomy Pictures Of The Day [Week 3/2010]](https://i.ytimg.com/vi/sqYS7W-kgL8/mqdefault.jpg "NASA Astronomy Pictures Of The Day [Week 3/2010]
http://facebook.com/ScienceReason ... NASA Astronomy Pictures Of The Day [Week 3/2010].
Please SUBSCRIBE to Science & Reason:
• http://www.youtube.com/Best0fScience
• http://www.youtube.com/ScienceTV
• http://www.youtube.com/FFreeThinker
• http://www.youtube.com/RationalHumanism
► Eclipse over the Temple of Poseidon
The Moon moved to partly block the Sun for a few minutes last week as a partial solar eclipse became momentarily visible across part of planet Earth. In the above single exposure image, meticulous planning enabled careful photographers to capture the partially eclipsed Sun well posed just above the ancient ruins of the Temple of Poseidon in Sounio, Greece.
• http://antwrp.gsfc.nasa.gov/apod/ap100118.html
► Dust Sculptures in the Rosette Nebula
Noted for the common beauty of its overall shape, parts of the Rosette Nebula, also known as NGC 2237, show beauty even when viewed up close. Visible above are globules of dark dust and gas that are slowly being eroded away by the energetic light and winds by nearby massive stars. Left alone long enough, the molecular-cloud globules would likely form stars and planets. The Rosette Nebula spans about 50 light-years across and lies about 4,500 light-years away.
• http://antwrp.gsfc.nasa.gov/apod/ap091202.html
► Watch Jupiter Rotate
What would it be like to coast by Jupiter and watch it rotate? This was just the experience of the New Horizons spacecraft as it approached and flew by Jupiter. Visible above in the extensive atmosphere of the Solar Systems largest planet are bands and belts of light and dark clouds, as well as giant rotating storm systems seen as ovals. The robotic New Horizons spacecraft continues to speed toward the outer Solar System and has recently passed the halfway point between Earth and Pluto.
• http://antwrp.gsfc.nasa.gov/apod/astropix.html
► NGC 6992: Filaments of the Veil Nebula
Wisps like this are all that remain visible of a Milky Way star. About 7,500 years ago that star exploded in a supernova leaving the Veil Nebula, also known as the Cygnus Loop. At the time, the expanding cloud was likely as bright as a crescent Moon, remaining visible for weeks to people living at the dawn of recorded history. Today, the resulting supernova remnant has faded.
• http://antwrp.gsfc.nasa.gov/apod/ap091201.html
► Dark Sand Cascades on Mars
They might look like trees on Mars, but theyre not. Groups of dark brown streaks have been photographed by the Mars Reconnaissance Orbiter on melting pinkish sand dunes covered with light frost. The image was taken near the North Pole of Mars. At that time, dark sand on the interior of Martian sand dunes became more and more visible as the spring Sun melted the lighter carbon dioxide ice. When occurring near the top of a dune, dark sand may cascade down the dune leaving dark surface streaks streaks that might appear at first to be trees standing in front of the lighter regions, but cast no shadows.
• http://antwrp.gsfc.nasa.gov/apod/ap100119.html
► Eclipses in the Shade
Eclipses are everywhere in this shady scene. The picture was taken on the Indian Ocean atoll island of Ellaidhoo, Maldives, in January 2010, during the longest annular solar eclipse for the next 1,000 years. Tall palm trees provided the shade. Their many crossed leaves created gaps that acted like pinhole cameras, scattering recognizable eclipse images across the white sands of a tropical garden near the beach. From this idyllic location near the centerline of the Moons shadow track, the ring of fire or annular phase of the eclipse lasted about 10 minutes and 55 seconds.
• http://antwrp.gsfc.nasa.gov/apod/ap100123.html
► Dust and the NGC 7771 Group
Some 200 million light-years distant toward the constellation Pegasus, NGC 7771 is the large, edge-on spiral near center, about 75,000 light-years across, with two smaller galaxies just below it. Large spiral NGC 7769 is seen face-on to the right. Galaxies of the NGC 7771 group are interacting, making repeated close passages that will ultimately result in galaxy-galaxy mergers on a cosmic timescale.
• http://antwrp.gsfc.nasa.gov/apod/ap100121.html
► Millennium Annular Solar Eclipse
The Moons shadow raced across planet Earth on January 15. Observers within the central shadow track were able to witness an annular solar eclipse as the Moons apparent size was too small to completely cover the Sun. A visually dramatic ring of fire, the annular phase lasted up to 11 minutes and 8 seconds depending on location, the longest annular solar eclipse for the next 1,000 years.
• http://antwrp.gsfc.nasa.gov/apod/ap100122.html
► Himalayan Skyscape
Capella, alpha star of the constellation Auriga, rises over Mt. Everest in this panoramic view of the top of the world at night.
• http://antwrp.gsfc.nasa.gov/apod/ap091205.html
.")
