This Month's Night Sky - NOTE: The next paragraph describes the sky as it appears at 10 pm EST (11 pm EDT) near mid- month. The sky also looks this way at 11 pm EST (midnight EDT) during the beginning of the month and at 9 pm EST (10 pm EDT) by month's end.
As the days lengthen, the stars of the Winter Triangle fade into evening's dusk. The "Big Dipper" asterism (Ursa Major) is well placed for viewing this month since it is almost directly overhead. Follow the curve of its handle to Arcturus (Bootes) and continue on the curve to Spica (Virgo). Regulus (Leo) is on the ecliptic (the path traced by the planets and Moon), just W. of overhead. Further W., on the ecliptic, find the Gemini Twins, Castor and Pollux, and finally the Pleiades asterism of Taurus.
MERCURY in the evening sky favors northern-based observers the first 2 weeks of the month. VENUS having plunged across the face of the Sun during inferior conjunction, emerges bruskly into the morning sky, rising higher as the month progresses. The planet will pass the asterism of the Circlet in Pisces, pause at a stationary point and resume prograde motion. Our sister planet will attain greatest illumination on the 30th. (mag. -4.7) MARS will spend the next couple months vanshing into the Sun to fulfill the appointment with superior conjunction on July 27 this year. Northern observers will have the best shot of catching MARS at sunset during the next few months.The brightest the red planet will shine is 1.5 mag, dimmer than the bright alpha star, Aldebaran, ruler of the Taurus constellation where Mars will remain until it nears conjunction. JUPITER is at opposition on April 8th. Now that Venus has passed into the morning sky, the giant planet will rule the night this Spring. SATURN rises earlier in the morning in Sagittarius, reaches a stationary point and begins retrograde motion on the 6th. URANUS is not visible this month.. The outer planet NEPTUNE rises in the morning sky.
Review how to determine Angular Measurement.
NOTE: For those observers not in the ET zone, convert the calendar times to your zone's time by subtracting one hour for CT, two for MT and three for PT. Don't forget to adjust for Daylight Savings Time when necessary by subtracting one hour from your planisphere's time. Dawn and dusk times must also be corrected. See your local newspaper, TV news, or cable TV's Weather Channel for sunrise and sunset times or check with the U.S. Naval observatory. Unfortunately some of these events may occur during daylight hours in your area.
|01||Aldebaran 0.3 deg S. of the Moon occultation from northeastern Africa, Arabiua, India, Mongolia, China, and Japan.|
|10||Jupiter 2 deg S. of Moon.|
Jupiter at Opposition (mag -2.5)
Regulus 0.7 of Moon, occultation from South Polynesia, Antarctica pennisula, and S. tip of South America.
|14||Uranus in conjunction with the Sun.|
|15||Moon at apogee.|
|16||Saturn 3 deg. S. of Moon.|
|20||Mercury at inferior conjunction.|
Lyrid Meteor Peak. Although the shower is generally fairly weak, it sometimes is surprising! Expect 20 meteors per hour during the peak at 12h UT.
Neptune .2 deg N. of Moon, occulatation from most of Australia, New Zealand, Melanesia, and central Polynesia.
|27||Moon at perigee.|
|28||Aldebaran 0.3 deg S. of the Moon occultation from North America, Cuba, eastern Canada, S. tip of Greenland, Europe, and N. Africa.|
|Phases of the Moon||Phase and Date(s)||Best viewed before local midnight|
|Deep Space Objects|
|Planets & Moon|
|Deep Space & Planets|
By now, many of the citizens of the U.S.A. have learned that a very rare phenomenon is about to grace the shores of the contiguous US states. The event is a total solar eclipse whose umbral path or moon shadow will cross about 3000 miles of the United States. Starting at the west coast, the shadow arrives in the late morning at the Pacific state of Oregon, races across fourteen US states, and plunges into the Atlantic by the southern state of South Carolina in the early afternoon, 4 hours 5 minutes and 47 seconds later. Totality will grace many National Parks and Monuments, various state capitals and major metropolitan areas as well as inaccessible mountain peaks. This is an event that Astra sincerely hopes will be seen by millions of her fellow citizens and visitors. The unbelievably beautiful and exciting total solar eclipse is almost guaranteed to spawn many new, young astronomers, and amateur observers. This eclipse umbral path will cover only landmasses in the continental US. This month's night sky article is about making daytime observations of the August 21, 2017 total solar eclipse.
So what is a total solar eclipse and how does it happen? A total solar eclipse happens during a new moon when the Moon and the Sun are perfectly aligned, darkness comes on Earth where ever the Moon's shadow falls. Have you ever noticed that the disk of the Sun and the Moon appear to be about the same size in the sky? The fact is they are very close. The Earth and the Moon are in orbit around the Sun, in addition the Moon is orbiting the Earth. Orbits are always ellipses, although some may be nearly circular. In an elliptical orbit, there are two points, one at the closest distance and another at the furthest. This means that the disks of the Moon and Sun are slightly larger at the close point (we use the term peri-), and slightly smaller at the far point (we call that ap-). In addition the Moon’s orbit is inclined to the ecliptic by 5 degrees, that is the plane of the Earth’s orbit about the Sun. This means that the Moon moves north and south in relation to the Earth's equator like a yo-yo on a string. Only when the Sun and the Moon are at the same point on the ecliptic (called nodes) can an eclipse occur.
Because all of the orbits are stable, this happens on a regular basis, about every 6 months, that is called an eclipse season. This means that there are approximately 2 eclipse seasons per year. A total solar eclipse occurs when the Moon is closest to the Earth, we use the term perigee. If the Moon is closer to apogee, a different kind of eclipse occurs; that is called an annular eclipse because the Sun appears as a ring and there is no total darkness. Whenever the Moon does not completely cover the disk of the Sun, it is called a partial eclipse. During any total eclipse localities not on the umbral path will see only a partial eclipse.
Darkness comes in daylight when the disk of the Sun is totally obscured, or eclipsed by the Moon. When the Moon's disk first covers the Sun, it is called first contact. As the eclipse progresses, the Earth below becomes cooler and the bright day continues to lose heat and intensity. Second contact comes at the beginning of totality. As the Moon covers the entire Sun, light begins to fade completely, the last point before total obscuration, the famous "Diamond Ring" effect appears, the only remaining spot of the Sun peaking from behind the lunar disk. Soon, only a thin edge of the Sun peaks through the mountainous terrain on the limb of the Moon, creating dots of light called "Baily's Beads". Second contact heralds totality. The Earth is plunged into darkness, now and only now, observers can stare directly at the disk of the Sun, er, um Moon. The Sun's chromosphere appears red, only briefly, and then the fantastic bellowing corona appears as a massive white mist shooting out from behind the Moon. Temperature of the gasses and ions in this white cloud is well over 1 million degrees. From the surface of the Sun, magenta prominences will spout past the lunar disk clearly visible to a ground-based telescope, now capable of imaging the eclipsed Sun without danger to observers or sensitive equipment. People and animals in the zone of totality become excited or confused. Devoted eclipse chasers give out a shout! All too soon, totality ends and once again eyes and instruments must be protected from the Sun's radiance.
OK, this is where Astras must warn folks: Please protect your eyes from exposure to the Sun! Check carefully any filter you use, including the cute cardboard eclipse glasses you just bought for a buck. The Sun can steal your vision, even if your eyes are not pained when you look through the filter. Make sure there are no pinholes. Also, while you are standing out in the summer sun for 2 or 3 hours, wear some sun screen, skin cancer is no joke. And remember: enjoy! enjoy! enjoy!
The August 21, 2017 total solar eclipse U.S.A. is the first total eclipse umbral path to reach any of the contiguous United States since February 26, 1979. The umbral path of that eclipse crossed only states in the northwest region of the country. This eclipse occurred during winter months and was clouded out for many locations. In 1991, the total solar eclipse umbral path crossed over the Pacific Ocean state of Hawaii. For both of these eclipses, sun chasers who were successful were willing to relocate to areas where viewing was possible. This year's eclipse is much more generous, crossing the length of the country. Please DO NOT miss viewing this eclipse if you are anywhere near the umbral path and make plans now to get to the path if you are not. Many eclipse-blessed locations have already filled up lodgings and sold out tickets to related events. For more information on this eclipse, check out Astra's Guide to the August 21, 2017 Total Solar Eclipse on this website.
--See You Under the Stars!
Astra for Astra's Almanac
The images above were created by Dawn Jenkins and are copyrighted. Please contact Astra at firstname.lastname@example.org if you wish to use them (especially the eclipse diagram) in another publication or website. Astra is open to sharing content with astronomical and educational organizations and individuals. The same applies to the text of the total solar eclipse featured article
This installment of "What's Up?" is ©2017 by Dawn Jenkins for Astra's Stargate. View Ron Leeseburg's Farewell Issue for information on where to find information such as is presented in this almanac.