Symbols of the Planets

The symbols of the eight planets, and Pluto, Credit: insightastrology.net

In our long history of staring up at the stars, human beings have assigned various qualities, names, and symbols for all the objects they have found there. Determined to find patterns in the heavens that might shed light on life here on Earth, many of these designations ascribed behavior to the celestial bodies.

When it comes to assigning signs to the planets, astrologists and astronomers – which were entwined disciplines in the past -made sure that these particular symbols were linked to the planets’ names or their history in some way.

Consider the planet Mercury, named after the Roman god who was himself the messenger of the gods, noted for his speed and swiftness. The name was assigned to this body largely because it is the planet closest to the Sun, and which therefore has the fastest rotation period. Hence, the symbol is meant to represent Mercury’s helmet and caduceus – a herald’s staff with snakes and wings intertwined.

Mercury, as imaged by the MESSENGER spacecraft, revealing parts of the never seen by human eyes. Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
Mercury, as imaged by the MESSENGER spacecraft, which was named after the messenger of the gods because it has the fastest orbit around the Sun. Image Credit: NASA/JHU/Carnegie Institution.

Venus:
Venus’ symbol has more than one meaning. Not only is it the sign for “female”, but it also represents the goddess Venus’ hand mirror. This representation of femininity makes sense considering Venus was the goddess of love and beauty. The symbol is also the chemical sign for copper; since copper was used to make mirrors in ancient times.

Earth:
Earth’s sign also has a variety of meanings, although it does not refer to a mythological god. The most popular view is that the circle with a cross in the middle represents the four main compass points.  It has also been interpreted as the Globus Cruciger, an old Christian symbol for Christ’s reign on Earth.

This symbol is not just limited to Christianity though, and has been used in various culture around the world. These include, but are not limited to,  Norse mythology (where it appears as the Solar or Odin’s Cross), Native American cultures (where it typically represented the four spirits of direction and the four sacred elements), the Celtic Cross, the Greek Cross, and the Egyptian Ankh.

In fact, perhaps owing to the simplicity of the design, cross-shaped incisions have made appearances as petroglyphs in European cult caves dating all the way back to the beginning of the Upper Paleolithic, and throughout prehistory to the Iron Age.

Mars, as photographed with the Mars Global Surveyor, is identified with the Roman god of war. Credit: NASA
Mars, as photographed with the Mars Global Surveyor, is identified with the Roman god of war. Credit: NASA

Mars:
Mars is named after the Roman god of war, owing perhaps to the planet’s reddish hue, which gives it the color of blood. For this reason, the symbol associated with Mars represents the god of wars’ shield and spear. Additionally, it is the same sign as the one used to represent “male”, and hence is associated with self-assertion, aggression, sexuality, energy, strength, ambition and impulsiveness.

Jupiter:
Jupiter’s sign, which looks like an ornate, oddly shaped “four,” also stands for a number of symbols. It has been said to represent an eagle, which is Jupiter’s bird. Additionally, the symbol can stand for a “Z,” which is the first letter of Zeus  – who was Jupiter’s Greek counterpart.

The line through the symbol is consistent with this, since it would indicate that it was an abbreviation for Zeus’ name. And last, but not least, there is the addition of the swirled line which is believed to represent a lighting bolt – which just happens to  Jupiter’s (and Zeus’) weapon of choice.

Saturn:
Like Jupiter, Saturn resembles another recognizable character – this time, it’s an “h.” However, this symbol is actually supposed to represent Saturn’s scythe or sickle, because Saturn is named after the Roman god of agriculture.

Jupiter's Great Red Spot and Ganymede's Shadow. Image Credit: NASA/ESA/A. Simon (Goddard Space Flight Center)
Jupiter, the largest planet in the Solar System, is appropriately named after the Roman father of the gods. Credit: NASA/ESA/A. Simon (Goddard Space Flight Center)

Uranus:
The sign for Uranus is a combination of two other signs – Mars’ sign and the symbol of the Sun – because the planet is connected to these two in mythology. Uranus represented heaven in Roman mythology, and this ancient civilization believed that the Sun’s light and Mars’ power ruled the heavens.

Neptune:
Neptune’s sign is linked to the sea god Neptune, who the planet was named after. Appropriately, the symbol represents this planet is in the shape of the sea god’s trident.

Pluto:
Although Pluto was demoted to a dwarf planet, it still has a symbol. Pluto’s sign is a combination of a “P” and a “L,” which are the first two letters in Pluto as well as the initials of Percival Lowell, the astronomer who discovered the planet.

Other Objects:
The Moon is represented by a crescent shape, which is a clear allusion to how the Moon appears in the night sky more often than not. Since the Moon is also tied to people’s perceptions, moods, and emotional make-up, the symbol has also come to represents the mind’s receptivity.

A full moon captured July 18, 2008. Credit: NASA/Sean Smith
A full moon captured July 18, 2008. Credit: NASA/Sean Smith

And then there’s the sun, which is represented by a circle with a dot in the middle. In the case of the Sun, this symbol represents the divine spirit (circle) surrounding the seed of potential, which is a direct association with ancient Sun worship and the central role Sun god’s played in ancient pantheons.

The planets have played an important role in the culture and astrological systems of every human culture. Because of this, the symbols, names, and terms that denote them continue to hold special significance in our hearts and minds.

We have many interesting articles on the planets here at Universe Today. For example, here is other articles including symbols of the planets and symbols of the Sun and Moon.

If you are looking for more information try signs of the planets and symbols of the minor planets.

Astronomy Cast has an episode on each planet including Saturn.

Universe Today has articles you will want to check out on symbols for the Sun and Moon and symbol for Earth.

If you are looking for more information, take a look at this website from NASA on the astronomical symbols or on the symbol for Pluto.

Astronomy Cast has an episode on each planet, so listen to all of them in order starting with Mercury.

Orbits of the Planets

Take a look at the Solar System from above, and you can see that the planets make nice circular orbits around the Sun. But dwarf planet’s Pluto’s orbit is very different. It’s highly elliptical, traveling around the Sun in a squashed circle. And Pluto’s orbit is highly inclined, traveling at an angle of 17-degrees. This strange orbit gives Pluto some unusual characteristics, sometimes bringing it within the orbit of Neptune. Credit: NASA

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Centuries ago, people believed that the Earth was the center of the Solar System. Slowly, that view was replaced with the heliocentric view. With that change came the realization that the planets orbit the Sun.

When Pluto was reclassified as a dwarf planet, Mercury became the planet with the most eccentric orbit. The eccentricity of an orbit is a measurement of how much the orbit deviates from a circular shape. If an orbit is a perfect circle, it has an eccentricity of zero, and that number increases with an increase in eccentricity. Mercury has an eccentricity of .21. Its orbit ranges from 46 million kilometers at the closest point to the Sun to 70 million kilometers at the farthest point. The closest point to the Sun in an orbit is called the perihelion, and the farthest point is the aphelion. Mercury is the fastest planet to orbit the Sun at approximately Earth 88 days.

Venus has the least eccentricity of any planet in our Solar System – eccentricity of .007 – with a nearly perfect circular orbit. Venus’ orbit ranges from 107 million kilometers at the perihelion to 109 million kilometers from the Sun. It takes 224.7 of our days to orbit the Sun. A day on Venus is actually longer than a year because the planet rotates so slowly. Seen from the Sun’s north pole, all of the planets rotate counter-clockwise, but Venus actually rotates clockwise; it is the only planet to do that.

Earth also has a very low eccentricity of .017. On average, the planet is about 150 million kilometers from the Sun, but it can range from 147 million kilometers to 152 million kilometers. It takes our planet roughly 365.256 days to orbit the Sun, which is the reason for leap years.

Mars has an eccentricity of .093 making it one of the most eccentric orbits in our Solar System. Mars perihelion is 207 million kilometers and its aphelion is 249 million kilometers from the Sun. Over time, Mars’ orbit has become more eccentric. It takes 687 Earth days to orbit the Sun.

Jupiter has an eccentricity of .048 with a perihelion of 741 million kilometers and an aphelion of 778 million kilometers. It takes 4331 Earth days – 11.86 of our years – for Jupiter to orbit the Sun.

Saturn has an eccentricity of .056. At its closest point, Saturn is 1.35 billion kilometers from the Sun, and 1.51 billion kilometers away at its farthest point. Depending on what position it is in its orbit, Saturn’s rings are fully visible or almost invisible. The planet takes 29.7 years to orbit the Sun. In fact, since it was discovered in 1610, Saturn has only orbited approximately 13 times. Earth has orbited the Sun almost 400 times since then.

Uranus has a perihelion of 2.75 billion kilometers and an aphelion of 3 billion kilometers from the Sun. Its eccentricity is .047. It takes Uranus 84.3 Earth years to orbit the Sun. Uranus is unique because it actually rotates on its side with an axial tilt of almost 99°.

Neptune’s eccentricity is .009, almost as low as Venus’. The planet has a perihelion of 4.45 billion kilometers and an aphelion of 4.55 billion kilometers. Since Pluto was reclassified as a dwarf planet, Neptune is the planet with an orbit farthest from the Sun.

Universe Today has articles on orbits of all the planets including Mercury and Mars.

There are a number of other sites, including one with animations of the orbits and what an orbit is.

Astronomy Cast has an episode on the orbit of the planets.

What are the Sizes of the Planets?

Size of the planets compared.

It is often difficult to grasp just how large the planets actually are. There are a number of ways to measure a planet, including diameter, volume, and surface area.

Mercury is the smallest planet in our Solar System since Pluto was demoted to a dwarf planet. It has a diameter of 4,879 km, and a surface area of 17.48 x 107 km2, which is only about 11% of Earth’s surface area. Mercury’s volume is even smaller in comparison at 6.083 x 1010 km3, which is only 5.4% the volume of Earth.

Venus is similar in size to Earth, which earned it the title of Earth’s twin. Venus has a diameter of 12,100 km and a surface area of 4.6 x 108 km2. These measurements are 95% and 90% of Earth’s diameter and surface area respectively. With a volume of 9.38 x 1011 km3, Venus’ volume is 86% of  Earth’s.

Earth has a diameter of 12,742 km and a surface area of 5.1 x 108 km2. Its volume of 1.08 x 1012 km3 gives the planet the largest volume of any of the terrestrial planets.

Mars is also a small planet, the second smallest in our Solar System. Mars’ diameter is 6,792 km, only about 53% of Earth’s diameter. At only 28% of Earth’s surface area, Mars has a very small surface area of 1.45 x 108 km2. Mars’ volume of 1.63 x 1011 km3 is only 15% of Earth’s volume.

All of the gas giants are larger in size than the four inner planets. Jupiter is the largest planet in our Solar System. It has a diameter of 143,000 km, which is more than 11 times the size of Earth’s diameter. The numbers only get larger from there. Jupiter has a surface area of 6.22 x 1010 km2. That is 122 times greater than Earth’s surface area. Jupiter’s volume of 1.43 x 1015 km3 is an incredible number. You can fit 1321 Earths inside Jupiter.

Saturn is the second largest planet in our Solar System. It has a diameter of 120,536 km across the equator, and a surface area of 4.27 x 1010 km2. With a volume of 8.27 x 1014 km3, Saturn can hold 764 Earths inside.

Uranus has a diameter of 51,118 km and a surface area of 8.1 x 109 km2. Although Uranus is much smaller than Jupiter, it is still large. With a volume of 6.83 x 1013 km3, you could fit 63 Earths inside the gas giant.

Neptune is slightly smaller than Uranus, but still very large. The planet has a diameter of 49,500 km. You could fit 57.7 Earths inside Neptune, which has a volume of 6.25 x1013 km3.  Neptune has a surface area of 7.64 x 109 km2, which is 15 times Earth’s surface area.

We have written many interesting articles about the Solar Planets here at Universe Today. Here’s tWhat are the Different Masses of the Planets?, What Is The Atmosphere Like On Other Planets?, What is the Average Surface Temperatures of the Planets? and What are the Diameters of the Planets?

For more information, check out this website to learn all about the planets and this page from NASA to learn about the planets.

Astronomy Cast has an episode on each of the planets including Mercury.

Carnival of Space #113: Extraterrestrial Impacts

This week’s Carnival of Space is hosted by Steinn at the Dynamics of Cats

Click here to read the Carnival of Space #113.

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Viewing the Jupiter Impact With Your Telescope

Are you ready to stay up a little late and see if you can catch the new dark spot on Jupiter from what could have either been an asteroid or comet impact? It happened somewhere between July 17th and 19th and the scar is still fresh and visible. However, there is just a little bit you need to know to make your viewing the Jupiter impact through your telescope a success.

By July 21, Joe Brimacombe was on this phenomena and recording it. Says Joe: “Got very lucky: CBET 1882 just announced a transient new black spot on Jupiter’s south polar region that it a probable comet impact. By chance I’d been imaging Jupiter between gaps in the clouds and seem to have captured it just before it rotated out of view. Seeing conditions were above average for Cairns.”

And he did a video for us:

Of course, Jupiter and its surface features are one of the easiest targets for backyard telescopes – so seeing something that large – and dark against a light background – should be easy. Right? Wrong. Viewing through our own Earth’s atmosphere plays a huge role on how we see the atmosphere of Jupiter. Low horizon conditions, unsteady or turbulent air, thin clouds, humidity, temperature… all of these are key factors in planetary observing. Observing skills come only with experience, but given the time and effort – you CAN do it!

1january03Before we go out to look for the impact, let’s stop and talk about Jupiter. There’s a reason so many amateurs love to this fast-rotating disk full of dynamic colored features… Because it’s so easy to see changes! Much like our own skin, the chemical composition of Jupiter’s atmosphere “tans” in the sunlight and the continual motion of its banded weather patterns keep an array of festoons, loops, ovals and barges on display at all times. How difficult is it to spot something? Then know this photo frame of a shadow transit is a 100% realistic view taken by me with a very small telescope with my camcorder. No tweaks, no filters… And it was much clearer to the eye than the camera. However, we need to remember that Jupiter rotates completely in about 10 hours, so a feature you see on its meridian at 11:00 pm won’t be there at 3:00 am. Like the “Great Red Spot”, the whole atmosphere is constantly on the move and there’s no guarantee that something that looks great one night will return again on another.

Now, let’s think positively! The impact spot is located near Jupiter’s System II longitude 210°. Although it’s small, if you use a lot of magnification, you should be able to spot it near the pole. The next thing you need to know is when to look! And here are the times the Jupiter impact can be seen for the next 10 days: July 25, 10:54 and 20:49; July 26, 6:45 and 16:41; July 27, 2:36, 12:32 and 22:27; July 28, 8:23 and 18:18; July 29, 4:14, 14:20 and 23:59; July 30, 10:01 and 19:56; July 31, 5:52 and 15:48. For August 1, 01:43, 11:39, 21:34; August 2, 7:32 and 17:25; August 3, 3:23, 13:17 and 23:12; August 4, 9:08 and 19:03; August 5, 4:59 and 14:54; August 6, 0:50, 10:46 and 20:41; August 7, 6:37 and 16:32; August 8, 2:28, 12:24 and 22:18; August 9, 8:15 and 18:20; August 10, 4:06, 14:01, 23:57; August 11, 9:53 and 19:48; August 12, 5:42 and 15:39; August 13, 01:35, 11:31 and 21:26; Auugst 14, 7:22 and 17:17; August 15, 3:13, 13:08, 23:04. Remember, these are very approximate Universal times when it should be visible on the meridian and you should have at least 20-30 minutes of opportunity on either side of the listed time to catch it as it rotates in and out.

Will the impact spot last in the days ahead? Unfortunately, just like the Shoemaker-Levy impact, the atmosphere will shred the debris cloud quickly. It is difficult enough to catch a feature near Jupiter’s poles because of limb darkening – so don’t wait to make your observations. Wishing you clear and steady skies!

Many thanks to Joe Brimacombe of Southern Galactic for sharing his incredible images with us!

Hubble Powers Up to Capture Jupiter Impact Site

This Hubble picture, taken on July 23, by the new Wide Field Camera 3, is the sharpest visible-light picture taken of the atmospheric debris from a comet or asteroid that collided with Jupiter on July 19. Credit: NASA, ESA, and H. Hammel (Space Science Institute, Boulder, Colo.), and the Jupiter Impact Team

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The Hubble Space Telescope was undergoing a thorough checkout of all its systems following the recent servicing mission, but scientists decided to drop everything and interrupt the observatory’s checkout and calibration to take an image of what every other telescope has by trying to view: the impact site on Jupiter. But Hubble does it better than anyone. This image, taken just yesterday (July 23) shows the black spot on the giant planet — created a small comet or asteroid — is expanding.

“Because we believe this magnitude of impact is rare, we are very fortunate to see it with Hubble,” said Amy Simon-Miller of NASA’s Goddard Space Flight Center in Greenbelt, Md. “Details seen in the Hubble view shows a lumpiness to the debris plume caused by turbulence in Jupiter’s atmosphere.”

The new Hubble images also confirm that the May servicing visit by space shuttle astronauts was a big success.

The Jupiter impact has been a sensation ever since Australian amateur astronomer Anthony Wesley imaged a black spot on the planet on July 19. , The only other time such a feature has been seen on Jupiter was 15 years ago after the collision of fragments from comet Shoemaker-Levy 9.

For the past several days, Earth-based telescopes have been trained on Jupiter. To capture the unfolding drama 360 million miles away, Matt Mountain, director of the Space Telescope Science Institute in Baltimore, gave observation time to a team of astronomers led by Heidi Hammel of the Space Science Institute in Boulder, Colo.

“Hubble’s truly exquisite imaging capability has revealed an astonishing wealth of detail in the impact site,” Hammel said. “By combining these images with our ground-based data at other wavelengths, our Hubble data will allow a comprehensive understanding of exactly what is happening to the impact debris.”

Simon-Miller estimated the diameter of the impacting object was the size of several football fields. The force of the explosion on Jupiter was thousands of times more powerful than the suspected comet or asteroid that exploded over the Siberian Tunguska River Valley in June 1908.

The image was taken with the Wide Field Camera 3. The new camera, installed by the astronauts aboard space shuttle Atlantis in May, is not yet fully calibrated. While it is possible to obtain celestial images, the camera’s full power has yet to be seen.

“This is just one example of what Hubble’s new, state-of-the-art camera can do, thanks to the STS-125 astronauts and the entire Hubble team,” said Ed Weiler, associate administrator of NASA’s Science Mission Directorate in Washington. “However, the best is yet to come.”

Source: NASA

Company Flies Biofuel Rocket (Video)

Flometrics, Inc. successfully flew a liquid fueled rocket with a 100% renewable fuel, a version of JP-8 (Jet Propellant 8) and liquid oxygen. The 180 lb (81 kg) rocket was 20 feet (6 meters) tall, 1 foot (.3 meters) diameter and it was powered by a RocketDyne LR-101 rocket engine that was originally used as a steering engine on the early Atlas and Delta rockets. The rocket performance during the 15 second long burn was better than the performance of a similar rocket using RP-1 refined kerosene rocket fuel. It reached an altitude of approximately 20,000 ft (6096 m) and may have exceeded Mach 1. The biofuel ran cleaner than the standard rocket fuel that has been used before. Since the biofuel was originally designed for jets, it may be possible to tune it for better performance in rocket engines. The fuel was developed by the Energy and Environment Research Center (EERC) at the University of North Dakota.

Source: Flometrics

Weekend SkyWatcher’s Forecast: July 24-26, 2009

Greetings, fellow SkyWatchers! Has everyone enjoyed the Apollo revival? I certainly have – and now the Moon is gently returning to evening sky and offering us great opportunities over the coming evenings to do a little bit of study with binoculars and telescopes. Look for its slender crescent just after sunset! This weekend we’re going to try an open cluster you may never have seen that works well for small optics and a Herschel object with a real twist. Need more? Then we’ll check out a beautifully colored double star, too… But not the one you expect! Grab your telescopes and binoculars and I’ll see you in the back yard…

delandresFriday, July 24, 2009 – Today let’s start with the 1853 birth on this date of Henri-Alexandre Deslandres. Do you recognize his name from our lunar studies? He invented the spectroheliograph to photograph the Sun in monochromatic light! Deslandres also observed the spectra of planets and stars and measured their radial velocities. Did you see the very young crescent of the Moon during twilight? The Moon played an important role in history on this date. The Apollo 11 astronauts splashed down from their return from the Moon on this date in 1969! Only 15 years before, in 1954, the sound of a human voice had been reflected off the Moon’s surface and returned to Earth. James H. Trexler at the Naval Research Laboratory spoke into a microphone at the laboratory’s Maryland facility, and the sound was relayed back 2.5 seconds later. Although ‘‘Operation Moon Bounce’’ was only a repetition of vowel sounds, Trexler felt the project held promise as a communications and radar intercept device. It might be worth it to point out that many radars are very close to the theoretical possibility of contacting the Moon, and hence the practicality of building a system capable of intercepting these systems by reflections from the Moon is not beyond the realm of possibility.

IC4665

Tonight we start with a group of young stars beginning their stellar evolution and end with an old solitary elder preparing to move onto an even ‘‘higher realm.’’ Open cluster IC 4665 is easily detected with just about any optical aid about a finger-width north-northeast of Beta Ophiuchi (RA 17 46 18 Dec +05 43 00). Discovered by Philippe Loys de Cheseaux in the mid-1700s, this 1,400 light year distant cluster consists of about 30 mixed-magnitude stars all less than 40 million years of age. Despite its early discovery, IC 4665 did not achieve broad enough recognition for Dreyer to include it in the late nineteenth-century New General Catalog (NGC), and it was later added as a supplement to the NGC in the Index Catalog of 1908. Be sure to use low power to see all of this large group.

Saturday, July 25, 2009 – Today we celebrate a success of the U.S.S.R. space program with the achievement of cosmonaut Svetlana Savitskaya, the first woman to walk in space (in 1982 on this date) and only the second female to go into space, preceding Sally Ride. Today is also the date of the 1973 launch of Soviet Mars 5 probe. Although it didn’t complete its full mission, it did send back 60 photos of the Martian Southern Hemisphere!

vendelinus

Although poor position makes study difficult during the first few lunar days, be sure to look for the ancient impact Vendelinus. Spanning 150 kilometers in diameter and with walls reaching up to 4,400 meters in height, lava flow has long ago eradicated any interior features. Its old walls hold mute testimony to later impact events such as crater Holden on the south shore, larger Lame on the northeast edge, and sharp Lohse northwest. Mark your challenge list!

ngc6401Tonight’s challenge is Herschel I.44, also known as NGC 6104, a 9.5-magnitude globular cluster around two finger-widths northeast of Theta Ophiuchi and a little more than a degree due east of star 51 (RA 17 38 37 Dec –23 54 31). Discovered by William Herschel in 1784 and often classed as ‘‘uncertain,’’ this halo object has been pegged by today’s powerful as a Class VIII and given a rough distance from the galactic center of 8,800 light-years. Although neither William nor John could resolve this globular and listed it originally as a bright nebula, studies in 1977 revealed a nearby suspected planetary nebula named Peterson 1. Thirteen years later, further study revealed this wasn’t a nebula at all but evidence of a symbiotic star. Symbiotic stars are a true rarity—not a single star at all but a binary system. A red giant dumps mass toward a white dwarf in the form of an accretion disk. When this reaches critical mass, it then causes a thermonuclear explosion, resulting in a planetary nebula. Although no evidence exists that this object is located within metal-rich NGC 6401, just being able to see it in the same field makes this journey both unique and exciting!

Sunday, July 26, 2009 – On this date in 1969 in a vacuum-sealed room, the very first sample return of Moon rocks was studied.

Our own vacuum of space awaits as we view the area around Mare Crisium to have a look at this month’s lunar challenge—Macrobius.

macrobius

You’ll find it just northwest of the Crisium shore. Spanning 64 kilometers in diameter, this Class I impact crater drops to a depth of nearly 3,600 meters—about the same as many of our Earthly mines. Its central peak rises to 1,100 meters and may be visible as a small speck inside the crater’s interior. Be sure to mark your lunar challenge lists, and look for other features you may have missed before!

Omicron_OphSince the moonlight will now begin to interfere with our globular cluster studies, let’s waive these for a while as we take a look at some of the region’s most beautiful stars. Tonight your goal is to locate Omicron Ophiuchi, about a finger-width northeast of Theta (RA 17 18 00 Dec –24 17 02). At a distance of 360 light-years, the Omicron system is easily split by even small telescopes. The primary star is slightly dimmer than magnitude 5 and appears yellow to the eye. The secondary is near 7th magnitude and tends to be more orange in color. This wonderful star is on many doubles’ observing lists, so be sure to note it!

Jup_by_Sean_09-07-21_03-46Are you wanting to keep an eye out for those dark markings of the Jupiter impact, too? Well, they’re there! Just remember if you’re new to astronomy that features on Jupiter rotate as the planet turns and we’re turning, too. Seeing the new “spots” requires some calculations and these areas will rotate into meridian view about 2 hours and 6 minutes after the Great Red Spot makes an appearance. Also remember that our own atmospheric seeing conditions play a great role as well! If it just so happens the dark spots will be making their appearance will Jupiter is still very low on the horizon, chances are your luck with seeing them in a small telescope won’t be high. But, don’t let that discourage you from looking! It doesn’t take long for a planet to rise to good observing height and the spots will stay visible for several hours as they rotate in and out on either side of your computed appearance time. (And don’t forget galiean moon shadow transits can also cause dark markings… but these will be very round!)

Until next week? Enjoy your observations and keep reaching for the stars!

This week’s awesome images are (in order of appearance): Henri Deslandres (historical image), IC 4665 (credit—Palomar Observatory, courtesy of Caltech), Vendelinus (credit—Alan Chu), NGC 6401 (credit—Palomar Observatory, courtesy of Caltech), Macrobius on the edge of Crisium (credit—Greg Konkel) Omicron Ophiuchi (credit—Palomar Observatory, courtesy of Caltech) and Jupiter (credit-Sky & Telescope: Sean Walker). We thank you so much!

Giant Soap Bubble In Space

The Cygnus Bubble. Credit: T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOAO/AURA/NSF

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What looks like a giant soap bubble or even perhaps just a water drop on a camera lens is actually a newly discovered planetary nebula. Dave Jurasevich of the Mount Wilson Observatory in California spotted the “Cygnus Bubble” while recording images of the region in July 2008. A few days later, amateur astronomers Mel Helm and Keith Quattrocchi also found it. Then, in 2009, the Kitt Peak Observatory pointed its 4-meter Mayall telescope at the object, and created the image above. Spectacular!

The bubble has been there awhile, and probably won’t “pop” anytime soon. The object was officially named PN G75.5+1.7 just last week. Astronomers have looked back at older images and found the object, just barely discernible in some images, such as this image below taken by Jurasevich.

Faint "Bubble" Nebula in Cygnus - Imaged on 05 July 2008 by Dave Jurasevich

A closer look at images from the second Palomar Sky Survey revealed it had the same size and brightness 16 years ago. Jurasevich thinks it was overlooked because it is very faint.

“It’s a beautiful example,” says Adam Frank of the University of Rochester, New York. “Spherical ones are very rare.” One explanation is that the image is looking down the throat of a typical cylindrical nebula. However, it is still remarkably symmetrical, Frank says.

For more about the history of observing this object, check out this post on Jurasevich’s Star Imager site.

Source: New Scientist

The Grand Canyon From Space

Grand Canyon from space. Click for larger version. Credit: ESA

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The Grand Canyon is an awesome sight on Earth — one of the seven natural wonders of the world – and it looks breathtaking from space, too. This image was taken by the Envisat satellite, showing canyon walls, rock structures, old lava flows, buttes, ravines, stair-step topography in hues of pink, violet and gray.

Also visible in the image are the Colorado Plateau (upper right corner), the Mogollon Plateau (dark area under Colorado Plateau), Lake Meade (Y-shaped water body left of the canyon), Las Vegas, Nevada (bright white and blue area left of Lake Meade) and the southern tip of Utah (upper left).

Although a number of processes combined to create the Grand Canyon, it was formed primarily by the eroding action of the Colorado River that began about six million years ago. Other contributing factors include volcanism, continental drift and the semiarid climate.

As water erosion sculpted this majestic showplace, it revealed layers and layers of exposed rocks that provide us with a profound record of geologic events. As some of Earth’s oldest rock lies at the bottom of the canyon, it is said to be 1800 meters and a billion years deep. It is about 443 km long and 8 to 29 km wide.

This image was acquired by Envisat’s Medium Resolution Imaging Spectrometer (MERIS) instrument on 10 May 2009, working in Full Resolution mode to provide a spatial resolution of 300 meters.

Source: ESA