aads

When is my earliest sunset?

Adrian Strand captured this photo on a beach in northwest England.

Adrian Strand captured this photo on a beach in northwest England.

The winter solstice is the shortest day. It offers the shortest period of daylight. But, unless you live close to the Arctic Circle or Antarctic Circle, your earliest sunsets aren’t on or even near the solstice itself. Instead, your earliest sunsets will come before the winter solstice. The exact date of earliest sunset depends on your latitude. If you live in the southernmost U.S., or a comparable latitude (say, around 25 or 26 degrees N. latitude), your earliest sunsets are in late November. If you’re farther north – say, around 40 degrees N. latitude – your earliest sunsets are in early to mid-December.

And if you live in the Southern Hemisphere, your earliest sunrises are coming around now. Southern Hemisphere? Click here.

Why isn’t the earliest sunset on the year’s shortest day? To understand it, try thinking about it in terms of solar noon or midday, the time midway between sunrise and sunset, when the sun reaches its highest point for the day.

A clock ticks off exactly 24 hours from one noon to the next. But the actual days – as measured by the spin of the Earth – are rarely exactly 24 hours long.

So the exact time of solar noon, as measured by Earth’s spin, shifts in a seasonal way. If you measured Earth’s spin from one solar noon to the next, you’d find that – around the time of the December solstice – the time period between consecutive solar noons is actually half a minute longer than 24 hours.

So – two weeks before the solstice, for example – the sun reaches its noontime position at 11:52 a.m. local standard time. Two weeks later – on the winter solstice – the sun reaches its noontime position at 11:59 a.m. That’s 7 minutes later.

The later clock time for solar noon also means a later clock time for sunrise and sunset.

The result: earlier sunsets before the winter solstice and increasingly later sunrises for a few weeks after the winter solstice.

The exact date of earliest sunset varies with latitude. But the sequence is always the same. For the Northern Hemisphere, earliest sunset in early December, winter solstice, latest sunrise in early January.

In early December, the Southern Hemisphere is approaching its summer solstice. Sunset on that part of Earth will continue coming later until early July. Photo of sunset with crepuscular rays by Phil Rettke Photography in Ipswich QLD Australia. Visit Phil Rettke on Facebook.

In early December, the Southern Hemisphere is approaching its summer solstice. Sunset on that part of Earth will continue coming later until early July. Photo of sunset with crepuscular rays by Phil Rettke Photography in Ipswich, Queensland, Australia.

Meanwhile, if you’re in the Southern Hemisphere, take nearly everything we say here and apply it to your winter solstice in June. For the Southern Hemisphere, the earliest sunsets come prior to the winter solstice, which is typically around June 21. The latest sunrises occur after the June winter solstice.

During the month of December, it’s nearly summer in the Southern Hemisphere; the summer solstice comes this month for that hemisphere. So sunsets and sunrises are shifting in a similar way. For both hemispheres, the sequence in summer is: earliest sunrises before the summer solstice, then the summer solstice itself, then latest sunsets after the summer solstice.

As always, things get tricky if you look closely. Assuming you’re at a mid-temperate latitude, the earliest sunset for the Northern Hemisphere – and earliest sunrise for the Southern Hemisphere – come about two weeks before the December solstice, and the latest sunrise/latest sunset happen about two weeks after.

But at the other end of the year, in June and July, the time period is not equivalent. Again assuming a mid-temperate latitude, the earliest sunrise for the Northern Hemisphere – and earliest sunset for the Southern Hemisphere – comes only about one week before the June solstice, and the latest sunset/latest sunrise happens about one week after.

The time difference is due to the fact that the December solstice occurs when Earth is near its perihelion – or closest point to the sun – around which time we’re moving fastest in orbit. Meanwhile, the June solstice occurs when Earth is near aphelion – our farthest point from the sun – around which time we’re moving at our slowest in orbit.

View larger. Computed position of the sun looking eastward at the same time each morning from the Northern Hemisphere. December solstice point at lower right and June solstice point at upper left. Solar days are longer than 24 hours long at the solstices, yet less than 24 hours long at the equinoxes. Roughly midway between a solstice and an equinox, or vice versa, the solar day is exactly 24 hours long.

View larger. Computed position of the sun looking eastward at the same time each morning from the Northern Hemisphere. December solstice point at lower right and June solstice point at upper left. Solar days are longer than 24 hours long at the solstices, yet less than 24 hours long at the equinoxes. Roughly midway between a solstice and an equinox, or vice versa, the solar day is exactly 24 hours long.

In short, the earliest sunset/winter solstice/latest sunrise and earliest sunrise/summer solstice/latest sunset phenomena are due to the fact that true solar days are longer than 24 hours long for several weeks before and after the solstices. At and around the solstices, the Earth must rotate farther on its axis for the sun to return to its daily noontime position, primarily because the sun is appreciably north or south of the Earth’s equator.

However, perihelion accentuates the effect around the December solstice, giving a day length of 24 hours 30 seconds. And aphelion lessens the effect around the June solstice, giving a day length of 24 hours 13 seconds.

Bottom line: The earliest sunsets and latest sunrises don’t come on the winter solstice, the shortest day of the year. Instead, earliest sunsets come some weeks before the winter solstice. Latest sunrises come some weeks after it.

Here are more details about the earliest sunsets.



from EarthSky http://ift.tt/1tNt1eN
Adrian Strand captured this photo on a beach in northwest England.

Adrian Strand captured this photo on a beach in northwest England.

The winter solstice is the shortest day. It offers the shortest period of daylight. But, unless you live close to the Arctic Circle or Antarctic Circle, your earliest sunsets aren’t on or even near the solstice itself. Instead, your earliest sunsets will come before the winter solstice. The exact date of earliest sunset depends on your latitude. If you live in the southernmost U.S., or a comparable latitude (say, around 25 or 26 degrees N. latitude), your earliest sunsets are in late November. If you’re farther north – say, around 40 degrees N. latitude – your earliest sunsets are in early to mid-December.

And if you live in the Southern Hemisphere, your earliest sunrises are coming around now. Southern Hemisphere? Click here.

Why isn’t the earliest sunset on the year’s shortest day? To understand it, try thinking about it in terms of solar noon or midday, the time midway between sunrise and sunset, when the sun reaches its highest point for the day.

A clock ticks off exactly 24 hours from one noon to the next. But the actual days – as measured by the spin of the Earth – are rarely exactly 24 hours long.

So the exact time of solar noon, as measured by Earth’s spin, shifts in a seasonal way. If you measured Earth’s spin from one solar noon to the next, you’d find that – around the time of the December solstice – the time period between consecutive solar noons is actually half a minute longer than 24 hours.

So – two weeks before the solstice, for example – the sun reaches its noontime position at 11:52 a.m. local standard time. Two weeks later – on the winter solstice – the sun reaches its noontime position at 11:59 a.m. That’s 7 minutes later.

The later clock time for solar noon also means a later clock time for sunrise and sunset.

The result: earlier sunsets before the winter solstice and increasingly later sunrises for a few weeks after the winter solstice.

The exact date of earliest sunset varies with latitude. But the sequence is always the same. For the Northern Hemisphere, earliest sunset in early December, winter solstice, latest sunrise in early January.

In early December, the Southern Hemisphere is approaching its summer solstice. Sunset on that part of Earth will continue coming later until early July. Photo of sunset with crepuscular rays by Phil Rettke Photography in Ipswich QLD Australia. Visit Phil Rettke on Facebook.

In early December, the Southern Hemisphere is approaching its summer solstice. Sunset on that part of Earth will continue coming later until early July. Photo of sunset with crepuscular rays by Phil Rettke Photography in Ipswich, Queensland, Australia.

Meanwhile, if you’re in the Southern Hemisphere, take nearly everything we say here and apply it to your winter solstice in June. For the Southern Hemisphere, the earliest sunsets come prior to the winter solstice, which is typically around June 21. The latest sunrises occur after the June winter solstice.

During the month of December, it’s nearly summer in the Southern Hemisphere; the summer solstice comes this month for that hemisphere. So sunsets and sunrises are shifting in a similar way. For both hemispheres, the sequence in summer is: earliest sunrises before the summer solstice, then the summer solstice itself, then latest sunsets after the summer solstice.

As always, things get tricky if you look closely. Assuming you’re at a mid-temperate latitude, the earliest sunset for the Northern Hemisphere – and earliest sunrise for the Southern Hemisphere – come about two weeks before the December solstice, and the latest sunrise/latest sunset happen about two weeks after.

But at the other end of the year, in June and July, the time period is not equivalent. Again assuming a mid-temperate latitude, the earliest sunrise for the Northern Hemisphere – and earliest sunset for the Southern Hemisphere – comes only about one week before the June solstice, and the latest sunset/latest sunrise happens about one week after.

The time difference is due to the fact that the December solstice occurs when Earth is near its perihelion – or closest point to the sun – around which time we’re moving fastest in orbit. Meanwhile, the June solstice occurs when Earth is near aphelion – our farthest point from the sun – around which time we’re moving at our slowest in orbit.

View larger. Computed position of the sun looking eastward at the same time each morning from the Northern Hemisphere. December solstice point at lower right and June solstice point at upper left. Solar days are longer than 24 hours long at the solstices, yet less than 24 hours long at the equinoxes. Roughly midway between a solstice and an equinox, or vice versa, the solar day is exactly 24 hours long.

View larger. Computed position of the sun looking eastward at the same time each morning from the Northern Hemisphere. December solstice point at lower right and June solstice point at upper left. Solar days are longer than 24 hours long at the solstices, yet less than 24 hours long at the equinoxes. Roughly midway between a solstice and an equinox, or vice versa, the solar day is exactly 24 hours long.

In short, the earliest sunset/winter solstice/latest sunrise and earliest sunrise/summer solstice/latest sunset phenomena are due to the fact that true solar days are longer than 24 hours long for several weeks before and after the solstices. At and around the solstices, the Earth must rotate farther on its axis for the sun to return to its daily noontime position, primarily because the sun is appreciably north or south of the Earth’s equator.

However, perihelion accentuates the effect around the December solstice, giving a day length of 24 hours 30 seconds. And aphelion lessens the effect around the June solstice, giving a day length of 24 hours 13 seconds.

Bottom line: The earliest sunsets and latest sunrises don’t come on the winter solstice, the shortest day of the year. Instead, earliest sunsets come some weeks before the winter solstice. Latest sunrises come some weeks after it.

Here are more details about the earliest sunsets.



from EarthSky http://ift.tt/1tNt1eN

Now we know Earth blocks neutrinos

A visual representation of one of the highest-energy neutrino detections, superimposed on a view of the IceCube Lab near Earth’s South Pole. Image via IceCube Collaboration/ Penn State.

It used to be said that neutrinos were massless and would pass through anything. But in recent years, scientists have realized that these strange particles – some of which were formed in the first second of the early universe, and which travel at the speed of light – are only practically massless. And now it’s been proven experimentally, by scientists working with data at the IceCube detector at Earth’s South Pole, that very energetic neutrinos can, in fact, be blocked. Doug Cowen at Penn State University was a collaborator on the study. He said:

This achievement is important because it shows, for the first time, that very-high-energy neutrinos can be absorbed by something — in this case, the Earth.

The results of this recent experiment were published in the online edition of the peer-reviewed journal Nature on November 22, 2017.

At the highest energies, neutrinos will be absorbed by Earth and will never make it to IceCube. Image via IceCube Collaboration.

The IceCube detector is an array of 5,160 basketball-sized sensors frozen deep within a cubic kilometer of very clear ice near the South Pole. The detector made the first detections of extremely-high-energy neutrinos in 2013, but a mystery remained about whether any kind of matter could truly stop a neutrino’s journey through space. Cowen said:

We knew that lower-energy neutrinos pass through just about anything, but although we had expected higher-energy neutrinos to be different, no previous experiments had been able to demonstrate convincingly that higher-energy neutrinos could be stopped by anything.

A statement from these scientists said:

The study … is based on one year of data from about 10,800 neutrino-related interactions, stemming from a natural supply of very energetic neutrinos from space that go through a thick and dense absorber: the Earth. The energy of the neutrinos was critical to the study, as higher energy neutrinos are more likely to interact with matter and be absorbed by the Earth.

Scientists found that there were fewer energetic neutrinos making it all the way through the Earth to the IceCube detector than from less obstructed paths, such as those coming in at near-horizontal trajectories.

The probability of neutrinos being absorbed by the Earth was consistent with expectations from the Standard Model of particle physics, which scientists use to explain the fundamental forces and particles in the universe.

Read more from the IceCube Collaboration.

The Standard Model predicts that the probability that a neutrino interacts with matter increases with energy. Thus the recent results from IceCube agrees with the Standard Model, for energies up to 980 TeV. New physics could show up as deviations to this prediction at higher energies. Image via IceCube Collaboration.

Bottom line: It used to be said that neutrinos would “pass through anything.” An experiment near the South Pole reveals how Earth blocks them.

Source: Measurement of the multi-TeV neutrino interaction cross-section with IceCube using Earth absorption



from EarthSky http://ift.tt/2iWor1u

A visual representation of one of the highest-energy neutrino detections, superimposed on a view of the IceCube Lab near Earth’s South Pole. Image via IceCube Collaboration/ Penn State.

It used to be said that neutrinos were massless and would pass through anything. But in recent years, scientists have realized that these strange particles – some of which were formed in the first second of the early universe, and which travel at the speed of light – are only practically massless. And now it’s been proven experimentally, by scientists working with data at the IceCube detector at Earth’s South Pole, that very energetic neutrinos can, in fact, be blocked. Doug Cowen at Penn State University was a collaborator on the study. He said:

This achievement is important because it shows, for the first time, that very-high-energy neutrinos can be absorbed by something — in this case, the Earth.

The results of this recent experiment were published in the online edition of the peer-reviewed journal Nature on November 22, 2017.

At the highest energies, neutrinos will be absorbed by Earth and will never make it to IceCube. Image via IceCube Collaboration.

The IceCube detector is an array of 5,160 basketball-sized sensors frozen deep within a cubic kilometer of very clear ice near the South Pole. The detector made the first detections of extremely-high-energy neutrinos in 2013, but a mystery remained about whether any kind of matter could truly stop a neutrino’s journey through space. Cowen said:

We knew that lower-energy neutrinos pass through just about anything, but although we had expected higher-energy neutrinos to be different, no previous experiments had been able to demonstrate convincingly that higher-energy neutrinos could be stopped by anything.

A statement from these scientists said:

The study … is based on one year of data from about 10,800 neutrino-related interactions, stemming from a natural supply of very energetic neutrinos from space that go through a thick and dense absorber: the Earth. The energy of the neutrinos was critical to the study, as higher energy neutrinos are more likely to interact with matter and be absorbed by the Earth.

Scientists found that there were fewer energetic neutrinos making it all the way through the Earth to the IceCube detector than from less obstructed paths, such as those coming in at near-horizontal trajectories.

The probability of neutrinos being absorbed by the Earth was consistent with expectations from the Standard Model of particle physics, which scientists use to explain the fundamental forces and particles in the universe.

Read more from the IceCube Collaboration.

The Standard Model predicts that the probability that a neutrino interacts with matter increases with energy. Thus the recent results from IceCube agrees with the Standard Model, for energies up to 980 TeV. New physics could show up as deviations to this prediction at higher energies. Image via IceCube Collaboration.

Bottom line: It used to be said that neutrinos would “pass through anything.” An experiment near the South Pole reveals how Earth blocks them.

Source: Measurement of the multi-TeV neutrino interaction cross-section with IceCube using Earth absorption



from EarthSky http://ift.tt/2iWor1u

Before you toss another thing in the trash, watch this video


Every day, the average American throws away about 4.4 pounds of waste, about the weight of one chihuahua. Multiple that by every day of the year and over 300 million Americans and you get 167,000,000 tons of trash a year — or the equivalent of 76 billion chihuahuas.

Meggie Stewart, a senior majoring in Environmental Sciences, did the math for her two-minute video about landfills (above) — the first place winner for the Emory Office of Sustainability Initiatives 2017 Waste Video Competition. Emory is striving to achieve zero landfill waste on campus, since landfills have negative social, economic and environmental impacts.

from eScienceCommons http://ift.tt/2A8DL4J

Every day, the average American throws away about 4.4 pounds of waste, about the weight of one chihuahua. Multiple that by every day of the year and over 300 million Americans and you get 167,000,000 tons of trash a year — or the equivalent of 76 billion chihuahuas.

Meggie Stewart, a senior majoring in Environmental Sciences, did the math for her two-minute video about landfills (above) — the first place winner for the Emory Office of Sustainability Initiatives 2017 Waste Video Competition. Emory is striving to achieve zero landfill waste on campus, since landfills have negative social, economic and environmental impacts.

from eScienceCommons http://ift.tt/2A8DL4J

Army Sensors Can Now Detect Aircraft Damage As It Happens

The discovery opens the door for onboard features that could immediately alert the flight crew on the state of structural damage like matrix cracking and delamination as they occur.

from http://ift.tt/2hVDojy
The discovery opens the door for onboard features that could immediately alert the flight crew on the state of structural damage like matrix cracking and delamination as they occur.

from http://ift.tt/2hVDojy

Astro festivals, star parties, workshops

North Carolina’s Fort Macon State Park host a monthly dark night astronomy program open to the public. With the help of the Crystal Coast Star Gazers Group, telescopes are set up for public viewing. In this photo, group member Fred Angeli”s headlamp leaves a streak of light as he approaches his ‘scope to focus on the night sky. Photo by Doug Waters.

Interested in astronomy, but not sure where to begin? A first step can be to seek out your local astronomy club. It consists of a roomful of willing and able amateur astronomers, whose telescopes may offer your first glimpse of the cosmos. The Astronomical League, an umbrella organization of 240 amateur astronomy clubs and societies in the U.S.

The Astronomical League also helps us create and maintain the list of events on this page. Click here to visit the Astronomical League’s website.

Know of an event that’s not on the list below? Contact us.

Do you have a great photo of a star party in your area? Submit here.

Looking for an astronomy club in your area? Click here.

Special thanks also to the Royal Astronomical Society of Canada for help with this list.

Jump below the photo for a list of upcoming events! If no web link is given, it’s because the information for the upcoming event hasn’t been posted yet. Check back.

Jim Elliott of Powell, Ohio, contributed this photo. He wrote:

Jim Elliott of Powell, Ohio, contributed this photo. He wrote: “The moon over Jupiter over Columbus, Ohio, at the OSU planetarium star party. April 16, 2016.”

Upcoming astronomy events …winter, 2018

February 3
Regional Gathering of Amateur Astronomers
(a.k.a. BoBfest) Catawba Science Center
Hickory, North Carolina
www.catawbasky.org

February 7–11
Orange Blossom Special International Star Party
Withlacoochee River Park
Dade City, Florida
http://ift.tt/1WnMXnm

Feb 12-18
Winter Star Party
Southern Cross Astronomical Society
Chiefland Astronomy Village (5450 NW 52nd Court Chiefland, Florida 32626)
http://ift.tt/2jrDU9A

March 3
TriStar 2018
Guilford Technical Community College
Greensboro Astronomy Club and the
Cline Observatory
Jamestown, North Carolina
observatory_gtcc.edu/tristar/

April 11–14
Mid-South Star Gaze and Astronomy Conference
French Camp, Mississippi
http://ift.tt/1KlyoA0

April 14–21
The OzSky Star Safari
(a.k.a. Deepest South Texas Star Safari)
Coonabarabran, New South Wales, Australia
www.ozsky.org

April 21–22
Northeast Astronomy Forum
Suffern, New York
http://ift.tt/1HMGVYK

Here is Dan Lewelyn at Deerlick Astronomy Village near Atlanta, Georgia. Photo by Dave Woolsteen.

Here is Dan Lewelyn at Deerlick Astronomy Village near Atlanta, Georgia. Photo by Dave Woolsteen.

Here's the Texas Star Party in 2009, one of the biggest such events of the year, drawing about 500 deep-sky enthusiasts and their telescopes to the Davis Mountains of West Texas. Image via Todd Hargis / Ron Ronhaar. Used with permission.

Texas Star Party, one of the biggest public astronomy events of each year, drawing about 500 deep-sky enthusiasts and their telescopes to the Davis Mountains of West Texas. Image used with permission, via Todd Hargis and Ron Ronhaar.

Bottom line: List of astronomy and night sky events for the public, for 2018, compiled in cooperation with the awesome Astronomical League. Join in, and have fun!



from EarthSky http://ift.tt/1UhrUpV

North Carolina’s Fort Macon State Park host a monthly dark night astronomy program open to the public. With the help of the Crystal Coast Star Gazers Group, telescopes are set up for public viewing. In this photo, group member Fred Angeli”s headlamp leaves a streak of light as he approaches his ‘scope to focus on the night sky. Photo by Doug Waters.

Interested in astronomy, but not sure where to begin? A first step can be to seek out your local astronomy club. It consists of a roomful of willing and able amateur astronomers, whose telescopes may offer your first glimpse of the cosmos. The Astronomical League, an umbrella organization of 240 amateur astronomy clubs and societies in the U.S.

The Astronomical League also helps us create and maintain the list of events on this page. Click here to visit the Astronomical League’s website.

Know of an event that’s not on the list below? Contact us.

Do you have a great photo of a star party in your area? Submit here.

Looking for an astronomy club in your area? Click here.

Special thanks also to the Royal Astronomical Society of Canada for help with this list.

Jump below the photo for a list of upcoming events! If no web link is given, it’s because the information for the upcoming event hasn’t been posted yet. Check back.

Jim Elliott of Powell, Ohio, contributed this photo. He wrote:

Jim Elliott of Powell, Ohio, contributed this photo. He wrote: “The moon over Jupiter over Columbus, Ohio, at the OSU planetarium star party. April 16, 2016.”

Upcoming astronomy events …winter, 2018

February 3
Regional Gathering of Amateur Astronomers
(a.k.a. BoBfest) Catawba Science Center
Hickory, North Carolina
www.catawbasky.org

February 7–11
Orange Blossom Special International Star Party
Withlacoochee River Park
Dade City, Florida
http://ift.tt/1WnMXnm

Feb 12-18
Winter Star Party
Southern Cross Astronomical Society
Chiefland Astronomy Village (5450 NW 52nd Court Chiefland, Florida 32626)
http://ift.tt/2jrDU9A

March 3
TriStar 2018
Guilford Technical Community College
Greensboro Astronomy Club and the
Cline Observatory
Jamestown, North Carolina
observatory_gtcc.edu/tristar/

April 11–14
Mid-South Star Gaze and Astronomy Conference
French Camp, Mississippi
http://ift.tt/1KlyoA0

April 14–21
The OzSky Star Safari
(a.k.a. Deepest South Texas Star Safari)
Coonabarabran, New South Wales, Australia
www.ozsky.org

April 21–22
Northeast Astronomy Forum
Suffern, New York
http://ift.tt/1HMGVYK

Here is Dan Lewelyn at Deerlick Astronomy Village near Atlanta, Georgia. Photo by Dave Woolsteen.

Here is Dan Lewelyn at Deerlick Astronomy Village near Atlanta, Georgia. Photo by Dave Woolsteen.

Here's the Texas Star Party in 2009, one of the biggest such events of the year, drawing about 500 deep-sky enthusiasts and their telescopes to the Davis Mountains of West Texas. Image via Todd Hargis / Ron Ronhaar. Used with permission.

Texas Star Party, one of the biggest public astronomy events of each year, drawing about 500 deep-sky enthusiasts and their telescopes to the Davis Mountains of West Texas. Image used with permission, via Todd Hargis and Ron Ronhaar.

Bottom line: List of astronomy and night sky events for the public, for 2018, compiled in cooperation with the awesome Astronomical League. Join in, and have fun!



from EarthSky http://ift.tt/1UhrUpV

Watch for Mars and Spica before dawn

In late November and early December, 2017, get up before morning dawn – say, around one and one-half hours before sunrise – to see the planet Mars pairing up with the bright star Spica, brightest star in the constellation Virgo, on the sky’s dome. Look east, and you can’t miss the dazzling planet Jupiter near the horizon. Mars and Spica are those two colorful starlike objects shining above Jupiter in the eastern, predawn sky.

As darkness gives way to dawn in late November and early December 2017, look also for the brilliant planet Venus near the eastern horizon. Venus, Jupiter and Mars (and it so happens, Spica) travel in our sky along the ecliptic, which is the plane of Earth’s orbit around the sun. Most planets and moons in our solar system move in this plane. And so – when you see them in the sky – most planets lie along this line across the sky, which is marked in green on our chart above.

By the way, please understand that our chart above is very fanciful. That’s because Mars is so faint that it’ll probably disappear from view by the time Venus rises into your sky.

If you see only 1 planet before dawn now, it’ll be Jupiter. Dennis Chabot of Posne Night Sky Astrophotography caught this photo of Jupiter on Saturday morning, November 25, 2017.

Mars and Spica should be close enough together to fit within the same binocular field for another week or so, at least. The actual conjunction date is November 29, 2017, when Mars passes some 3O north of Spica on our sky’s dome. Three degrees in the sky is approximately the width of your thumb at an arm’s length.

Spica, the brighter of these two starlike points of light, radiates blue-white while Mars glowers with a reddish hue. If you have difficulty discerning the contrasting colors of these close-knit celestial gems with the eye alone, try viewing them through binoculars.

At present, Mars resides in front of Spica’s constellation, Virgo, while Jupiter shines in front of the constellation Libra. Relative to the backdrop stars of the zodiac, both Mars are Jupiter are going eastward day by day. Mars is going eastward through Virgo, toward Jupiter, and Jupiter is going eastward through Libra, away from Spica and Mars.

However, Mars travels much more quickly through the constellations of the zodiac than Jupiter does. In the morning sky on January 7, 2018, Mars will finally catch up with Jupiter in front of the constellation Libra. It’ll be a stunning conjunction, with Mars passing less than one-quarter degree (0.25o = half the moon’s diameter) south of Jupiter on the sky’s dome.

And it’ll be a great time to note the contrast in the brightness of Jupiter and Mars … so that you can watch Mars brighten to around Jupiter’s brightness as 2018 progresses!

In fact, 2018 will be be the best year in many years to see Mars.

Bottom line: Now the view toward the east before dawn has entirely changed. Bright Jupiter is the 1st object you’ll notice. Venus can only be seen very shortly before sunup. Mars and Spica are fainter, but close!



from EarthSky http://ift.tt/2z35Bz4

In late November and early December, 2017, get up before morning dawn – say, around one and one-half hours before sunrise – to see the planet Mars pairing up with the bright star Spica, brightest star in the constellation Virgo, on the sky’s dome. Look east, and you can’t miss the dazzling planet Jupiter near the horizon. Mars and Spica are those two colorful starlike objects shining above Jupiter in the eastern, predawn sky.

As darkness gives way to dawn in late November and early December 2017, look also for the brilliant planet Venus near the eastern horizon. Venus, Jupiter and Mars (and it so happens, Spica) travel in our sky along the ecliptic, which is the plane of Earth’s orbit around the sun. Most planets and moons in our solar system move in this plane. And so – when you see them in the sky – most planets lie along this line across the sky, which is marked in green on our chart above.

By the way, please understand that our chart above is very fanciful. That’s because Mars is so faint that it’ll probably disappear from view by the time Venus rises into your sky.

If you see only 1 planet before dawn now, it’ll be Jupiter. Dennis Chabot of Posne Night Sky Astrophotography caught this photo of Jupiter on Saturday morning, November 25, 2017.

Mars and Spica should be close enough together to fit within the same binocular field for another week or so, at least. The actual conjunction date is November 29, 2017, when Mars passes some 3O north of Spica on our sky’s dome. Three degrees in the sky is approximately the width of your thumb at an arm’s length.

Spica, the brighter of these two starlike points of light, radiates blue-white while Mars glowers with a reddish hue. If you have difficulty discerning the contrasting colors of these close-knit celestial gems with the eye alone, try viewing them through binoculars.

At present, Mars resides in front of Spica’s constellation, Virgo, while Jupiter shines in front of the constellation Libra. Relative to the backdrop stars of the zodiac, both Mars are Jupiter are going eastward day by day. Mars is going eastward through Virgo, toward Jupiter, and Jupiter is going eastward through Libra, away from Spica and Mars.

However, Mars travels much more quickly through the constellations of the zodiac than Jupiter does. In the morning sky on January 7, 2018, Mars will finally catch up with Jupiter in front of the constellation Libra. It’ll be a stunning conjunction, with Mars passing less than one-quarter degree (0.25o = half the moon’s diameter) south of Jupiter on the sky’s dome.

And it’ll be a great time to note the contrast in the brightness of Jupiter and Mars … so that you can watch Mars brighten to around Jupiter’s brightness as 2018 progresses!

In fact, 2018 will be be the best year in many years to see Mars.

Bottom line: Now the view toward the east before dawn has entirely changed. Bright Jupiter is the 1st object you’ll notice. Venus can only be seen very shortly before sunup. Mars and Spica are fainter, but close!



from EarthSky http://ift.tt/2z35Bz4

Birdseye view of iceberg A-68A

NASA’s Operation IceBridge, now in its ninth year, is an airborne mission flown annually over both polar regions to map the ice. A few flights during the 2017 campaign took scientists and instruments over Antarctica’s newly reshaped Larsen C ice shelf.

One of the big changes the scientists observed was the calving of an iceberg from the Larsen C ice shelf. Nathan Kurtz, IceBridge project scientist, said in a statement:

We observed the crack across the shelf during the campaign last year; it has since broken through and produced a huge iceberg.

The iceberg from Larsen C, named A-68A, was photographed during a flight on November 12, 2017. The photo above was acquired by the Digital Mapping System (DMS), which as essentially a downward-looking digital camera pointed out a window on the belly of the aircraft. This image shows part of the giant iceberg’s edge (the side closest to the shelf) and open water.

Scientists estimate that the edges of the shelf and iceberg tower about 100 feet (30 meters) above the surface of the sea. Some mélange – a mix of ice types – appears attached to the iceberg, and blocks of ice have fallen away, giving the berg’s edge giving it an angular appearance.

John Sonntag, IceBridge mission scientist, shot this photo from a window of the P-3 research plane. The flight aimed to get a better understanding the Larsen system as a whole, and scientists made gravity measurements to “see” the shape of the seafloor and bedrock below the ice. Read more in this blog post. Photo via NASA/John Sonntag.

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Bottom line: Photos of giant iceberg A-68A, that calved from Antarctica’s Larsen C ice shelf.

Read more from NASA’s Earth Observatory



from EarthSky http://ift.tt/2jp4r7j

NASA’s Operation IceBridge, now in its ninth year, is an airborne mission flown annually over both polar regions to map the ice. A few flights during the 2017 campaign took scientists and instruments over Antarctica’s newly reshaped Larsen C ice shelf.

One of the big changes the scientists observed was the calving of an iceberg from the Larsen C ice shelf. Nathan Kurtz, IceBridge project scientist, said in a statement:

We observed the crack across the shelf during the campaign last year; it has since broken through and produced a huge iceberg.

The iceberg from Larsen C, named A-68A, was photographed during a flight on November 12, 2017. The photo above was acquired by the Digital Mapping System (DMS), which as essentially a downward-looking digital camera pointed out a window on the belly of the aircraft. This image shows part of the giant iceberg’s edge (the side closest to the shelf) and open water.

Scientists estimate that the edges of the shelf and iceberg tower about 100 feet (30 meters) above the surface of the sea. Some mélange – a mix of ice types – appears attached to the iceberg, and blocks of ice have fallen away, giving the berg’s edge giving it an angular appearance.

John Sonntag, IceBridge mission scientist, shot this photo from a window of the P-3 research plane. The flight aimed to get a better understanding the Larsen system as a whole, and scientists made gravity measurements to “see” the shape of the seafloor and bedrock below the ice. Read more in this blog post. Photo via NASA/John Sonntag.

Enjoying EarthSky so far? Sign up for our free daily newsletter today!

Donate to EarthSky: Your support means the world to us

Bottom line: Photos of giant iceberg A-68A, that calved from Antarctica’s Larsen C ice shelf.

Read more from NASA’s Earth Observatory



from EarthSky http://ift.tt/2jp4r7j

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