Give the Orion Parsec 8300C, a try, and see if you still look at your DSLR camera
Astronomy Products – The Orion Parsec 8300C is the latest CCD time-machine-to-the-stars capable of taking one-shot, full-frame, 8.3-megapixel color views during your “Journey to the Beginning of Space and Time” in perfect resolution. The Orion Parsec 8300C Astronomical Imaging Camera is designed and engineered around Kodak’s 8.3-megapixel KAF-8300 sensor and is one of the most advanced CCD time-machines-to-the-stars you can purchase to “Journey to the Beginning of Space and Time.
Amazing color images of the universe
The Orion Parsec 8300C Astronomical Imaging Camera’s color Kodak CCD chip is built around the 5.4 micron x 5.4-micron pixel size for superior resolution and uses Kodak’s microlens technology for maximum sensitivity. Regulated dual-stage thermoelectric cooling and the adjustable fan included with the Orion Parsec 8300C Astronomical Imaging Camera reduces the thermal noise you’ll experience while the internal full-frame memory buffer allows you to reliably and efficiently download your images for later use.
Top quality at a reasonable price
You get all of this Astro imaging power at a relatively low price, considering the quality of the views this outstanding CCD camera produces, and the Parsec 8300C Astronomical Imaging Camera is compatible with Windows XP and later operating systems. You just plug the Parsec 8300C Astronomical Imaging Camera into the USB 2.0 port on your computer with the included cable and power your time-machine-to-the-stars using the 12-volt DC power cable included that plugs into a car accessory jack, or other compatible power sources.
Human beings were designed to view the universe using two eyes
Astronomical binoculars are a time-machine-to-the-stars that will make your “Journey to the Beginning of Space and Time” a trip of a lifetime. The views you’ll experience during your journey will blow-your-mind using two eyes, rather than one, and you’ll return from your trip with tales of space and time your astronomy buddies will envy. The Orion BT100 Premium Binocular Telescope’s 100mm aperture helps to create bright, high-contrast 90 degree views of the universe at 24x magnification, using included 25mm Sirius Plossl eyepieces, that both your eyes will love.
Astronomical binocular telescope with amazing image quality
A 4-inch refractor that accepts standard 1 1/4 eyepieces that are focused individually for optimal performance, the Orion BT100 Premium Binocular Telescope features an all-metal body, fully multicoated achromatic objective lenses, Porro prisms made of BaK-4 glass, and removable eyepieces. Just mount your two-eyed time-machine-to-the-stars on a sturdy heavy-duty tripod, which isn’t included, slip the 25mm Sirius Plossl eyepieces into place in the integrated 90 degree prism assemblies, and blast-off from the Earth and “Journey to the beginning of Space and Time” to experience the wonders of the universe through two eyes.
Blast off to the stars with the Orion BT100 Binocular telescope
Flip the switch on your Meade LS-6 and being your “Journey to the Beginning of Space and Time”
Astronomy Products – Just set up your time-machine-to-the-stars, flick the ignition switch, and your “Journey to the Beginning of Space and Time” begins. Incorporating GPS satellites, internal leveling sensors, a magnetic north compass, and a built-in ECLIPS CCD imager capable of displaying vibrant astroimages on the scope or filing them away so you can send them to all of your astronomy buddies, later, the Meade LS-6 ACF Telescope includes the industry’s most advanced go-to astronomy system, for truly hands-free star-gazing.
Flick the switch, connect to GPS
The Light Switch Technology included with the Meade LS-6 go-to telescope goes to work with the flick of the switch, turning over the job of connecting the global positioning system with overhead satellites to a built-in Integrated Sensor Module (ISM). The global positioning system pinpoints the exact location and local time of your time-machine-to-the-stars on the planet’s surface and then the Level North Technology sensors silently search for two alignment stars and automatically start charting out a real-time sky map of the night sky in its memory banks for the present time and your location on the Earth’s surface.
The perfect telescope for the educated amateur astronomer heading out into the universe for their first “Journey to the Beginning of Space and Time”. The Meade LS-6 will automatically take you to points in space and time you’ll never forget and you can take a few pictures of your unforgettable views to show your friends, when you get back.
Perfect telescope for both amateur and professional astronomers
Experienced astronomers will love not having to remember the name of alignment stars or having to worry about the view being blocked by a tree or house, which can be frustrating and time-consuming to solve. The Meade LS-6 go-to telescope solves these problems and gives you more time for what you really want to do, “Journey to the Beginning of Space and Time”.
A lightweight and portable observatory you can set up anywhere
Astronomy Products – Kendrick Astro Instruments has been in the business of selling some of the top observer tents in the world for years. Stargazers love the ease of use and set up of Kendrick observer tents, but nothing is perfect, and Kendrick has been listening to its customers. Measuring 10 feet wide by 15 feet long and 6.5 feet high at the center, Kendrick Astro Instruments Stargate Observer Tent is the latest edition to Kendrick’s line of observer tents introduced a decade ago. Still including everything you loved about Kendrick’s original Observatory Tent, the new Kendrick Astro Instruments Stargate Observer Tent has been redesigned to include two separate rooms, one for you to continue your “Journey to the Beginning of Space and Time, and another for sleeping away the hours, separated by a polyester wall.
Great for the amateur or professional astronomer
You set up your time-machine-to-the-stars in the 10 foot x 9 foot star-gazing room, and then you and your weary-eyed stargazing companion sleep away the hours of the day in the smaller 10 foot x 6-foot sleeping area. Once the sun goes down and the stars appear in the night sky, you simply head into your observatory and unzip the 6-foot-wide observing flap, and continue your “Journey to the Beginning of Space and Time” in perfect comfort. Once you return from your adventure, simply close the observing flap, cover your telescope, and move into the next room for some well-deserved rest.
Grab Kendrick Astro Instrument’s Stargate Observer Tent and let your journey to the beginning of space and time continue
Astronomy News – Supernovas are some of the most powerful and visually striking events observed during the human “Journey to the Beginning of Space and Time. Releasing more energy in a single moment than Sol will over its entire lifetime, a supernova is luminous enough to shine brighter in the night sky than entire galaxies during one moment in space and time, before slowly fading from view over several weeks or months. The force of a supernova expels a large percentage of a star’s mass into the darkness of space and time at about 10 percent of the speed of light and creates a shock wave that sweeps up the expanding shell of gas and dust released during the explosion referred to by astronomers as a supernova remnant.
Astronomers search for new supernovae
Astronomers using NASA’s Spitzer Space Telescope to search the night sky for active galactic nuclei (AGN), super-massive black holes at the center of galaxies, recently reported the discovery of a supernova smothered in the remnants of its own star-dust during their search. This has astronomers scratching their heads in amazement at something they have never viewed during the human “Journey to the Beginning of Space and Time. Scientists think supernovas like this one probably occurred during the early universe, more than they do during present time, and this discovery has astronomers looking for answers to questions they never thought they would be asking.
Astronomers realised something was different
The recorded temperature of the object they were viewing was about 1,000 Kelvin (about 700 degrees Celsius), which is slightly hotter than the surface of Venus. This means something was dissipating the light energy of the supernova as heat? Astronomers wondered if the dust from the supernova could be choking off the light from the supernova and creating the heat they were viewing? Taking data from studies of NASA’s Spitzer Space Telescope astronomers worked backward in space and time to see if they could figure out what kind of star could have theoretically created this supernova and if they could recreate a scenario where the dust from a supernova obscures the universe from the light released during the supernova. They calculated that the star in this supernova would have to be a giant star at least 50 times as massive as Sol. Astronomers have viewed these types of stars releasing huge clouds of dust as they near the end of their lives, but they calculated this particular star probably released clouds of stardust several times during this same period of time. The last cloud of stardust expelled would, therefore, be closer to this massive star, than earlier released clouds of stardust, they reasoned. If the earlier dust cloud was also opaque, it would absorb the light energy released during later energy releases, and this could certainly account for the hot dust cloud they observed through NASA’s Spitzer Space Telescope.
Six exo-planets are circling red dwarf star Gliese 581 20 light-years distant in the constellation Libra
Astronomy News – The human search for an exoplanet capable of being a cradle for a new human genesis found what many consider the first exoplanet with the physical makeup to make it possible. A team of planet hunters from the University of California (UC) Santa Cruz and the Carnegie Institute of Washington recently announced to the world the discovery of an exoplanet they believe has a few characteristics of an exoplanet with the right stuff to make life possible. Gliese 581g, as it’s referred too, has about three times the mass of Earth and appears to be situated in the right spot in the solar system of the red dwarf star Gliese 581 for the ingredients of life to exist. This is about dead center in what planet scientists term the habitable zone of Gliese 581, a position planet scientists believe could make it possible for water and an atmosphere to exist on this exoplanet, necessary ingredients for the formation of life, planet scientists believe.
Astronomers search for a cradle for a new human genesis
These planet hunters have been using one of the largest time-machine-to-the-stars on the planet, the Keck I Telescope in Hawaii’s W.M Keck Observatory, to journey 20 light years to the constellation of Libra to continue the search for more planets circling red dwarf star Gliese 581 that could be habitable. Planet hunters have been using the HIRES spectrometer to precisely measure the radial velocity of the host star – the motion of the star along the line of sight from Earth – and stars close to red dwarf star Gliese 581, in order to try to find other planets circling this red dwarf star. The gravitational pull of orbiting planets causes periodic changes in the radial velocity of the host star that astronomers can calculate using sophisticated mathematical techniques we’ll cover on another day. These are the techniques planet hunters used in order to find all of the stars they have found circling red dwarf star Gliese 581, which after the two most recent planet discoveries, brings the total to six exoplanets circling this distant star.
Astronomers believe Gliese 581g is in the habitable zone of its home star
The discovery of six exoplanets circling red dwarf star Gliese 581 marks the high-planet mark for the human hunt for planets capable of being a cradle for a new human genesis. Gliese 581g is the only planet of the six exoplanets discovered that astronomers have indicated, so far, as being in the life zone of the red dwarf star Gliese 581. This exoplanet orbits its parent star in about 37 days and measurements planet scientists have made of its mass indicates it’s probably a rocky planet with a definite surface and enough gravity to hang onto an atmosphere. Gliese 581g is also tidally locked to its parent star, which means that one side of the planet is always facing its host star and in perpetual daylight. This makes some planet scientists believe that the best place for life to exist would be in the terminator, the part of the planet between the day and night sides of the planet.
Astronomy News – The human “Journey to the Beginning of Space and Time’ discovered another neutron star on June 5, 2009, that’s currently keeping astronomers and space scientists busy looking into the unusual properties of this newest member of the pulsar zoo. Astronomers using NASA’s Chandra, Swift and Rossi X-ray observatories, the Fermi Gamma-ray Space Telescope and ESA’s XMM-Newton telescope have been taking a look at this slowly rotating neutron star with an ordinary surface magnetic field as it gives off x-rays and gamma rays. Astronomers think the facts they have collected during their study of neutron star SGR 0418+5729 could indicate the presence of an internal magnetic field much more powerful than the surface magnetic field of this pulsar. This has definite implications in relation to the evolution of the most powerful magnets we have observed during the human “Journey to the Beginning of Space and Time” and astronomers are now delving into the mysteries they see within this neutron star to determine the facts.
Another strange neutron star
Astronomers looking at neutron star SGR 0418+5729 think this pulsar is one of a strange breed of neutron stars they refer too as magnetars, which normally have strong to extreme magnetic fields 20 to 100 times above the average for galactic radio pulsars they have viewed in the universe. What really has astronomers viewing SGR 0418+5729 scratching their heads is the fact that over a 490 day period of observing this pulsar astronomers saw no detectable decrease in this neutron stars rotational rate.
Astronomers think that the lack of rotational slowing of this neutron star could mean that the radiation of low-frequency waves is pretty weak, which leads them to believe the surface magnetic field of this pulsar must be quite a bit less powerful than normal. This conclusion gives astronomers another puzzle to solve, since with this thought astronomers are wondering where the energy for this neutron stars power bursts and x-ray emissions come from.
Does the power and energy creating this neutron stars power bursts and x-ray emissions originate in the twisting and amplifying of this pulsars internal magnetic field in the chaotic interior of this neutron star?
Present theories on this indicate that astronomers believe that if the internal magnetic field becomes ten or more times stronger than the surface magnetic field, the twisting or decay of the magnetic field could lead to the production of steady and bursting x-rays through the heating of the pulsar’s crust or the acceleration of particles in the magnetic field.
The question astronomers want to answer now is how large can the imbalance between the surface and interior magnetic fields be? If further observations indicate that the surface magnetic field limit is pushed too low, then astronomers will have to dig a little deeper into SGR 0418+5729 to find out why this neutron star is rotating slower.
The energy of the sun affects all life on Earth in ways we don’t even imagine
Humans have worshipped Sol for thousands of years
The original source of energy for all life on Earth, Sol has always ruled the lives and minds of human beings in many ways. The ruler of the daytime sky in ancient times and still today, Sol was worshipped by ancient humans of many cultures, and will always be a major force in the life of every human being on Earth. The Sumerians worshiped Utu as their sun god over two thousand years ago and modern humans worship the sun in their own way. We send spacecraft toward Sol, to study the lifecycle and physical and chemical characteristics of our sun, and determine everything we can about the sun.
Astronomy News – Hinode (Solar-B) is one spacecraft humans have sent out toward Sol in an attempt to delve deeper into the mysteries of the sun. A highly sophisticated observational satellite equipped with three solar telescopes, Hinode has recently revealed that the solar corona isn’t quite as static as solar scientists were first thinking. Hinode has surprised solar scientists of late with views of complex structures in the solar chromosphere, solar scientists use to think were static, but now believe to be dynamic structures flowing in time. This is making solar scientists rethink some of the previous ideas they had about the heating mechanisms and dynamics of the active solar corona.
Astronomers study the Sun continuously in an attempt to understand its mysteries
What questions will solar scientists working with Hinode try to answer next? They’ll be looking into why a hot corona exists above a cooler atmosphere? The origins and driving forces behind solar flares and the Sol’s magnetic field? The changes that the release of solar energy in its many forms has on interplanetary space in our solar system and life on Earth? The answers to these questions could be a key to eventually answering many of the questions the first stargazers and all humans have been asking for thousands of years. Solar scientists are also interested in knowing how magnetic changes near Sol’s surface effect the heliosphere, the outer atmosphere of Sol that extends beyond Pluto, and how severe changes in the heliosphere can cause satellites to malfunction and electrical blackouts on Earth.
Stargazers Halloween treats abound in autumn’s night sky
Winter treat for the lonely wanderer
Astronomy news (2013-10-15) – Cassiopeia the Queen is one of the first northern deep sky objects we’ll view during our “Journey to the Beginning of Space and Time”. Cassiopeia the Queen is easily recognizable in autumn’s night sky using her characteristic W or M shape form and she was one of the 48 constellations originally listed by the 2nd-century Greek astronomer Ptolemy during his observations of the night sky. Today, Cassiopeia the Queen is one of 88 constellations recognized by modern stargazers in the night sky, and the abundance of magnificent open star clusters within her arms provides viewers with a chance to see a variety of outstanding celestial objects that have been entertaining stargazers for thousands of years.
Cassiopeia the Queen is a familiar sight for modern astronomers and stargazers in the mid-northern latitudes of planet Earth and is often one of the first constellations in the northern sky beginning stargazers journey to view. Board your time-machine-to-the-stars near the end of October, or the beginning of November, and take the family on a journey through time and space to visit Cassiopeia the Queen. A visit with Cassiopeia the Queen will open a child’s mind to the possibilities of the universe, before them, and your wife will be able to tell her friends that you took her out last night.
Both astronomers and ancient navigators used Cassiopeia as a guide to finding their way
One of the best open star clusters you can view with the naked eye is 6.5 magnitude NGC 129, a large, bright, open cluster of stars 8×50 astronomical binoculars will reveal to have six to twelve brighter stars nestled within the collective glow of a field of stars too faint to resolve using binoculars. You should see about 35 celestial bodies in this region of space and time 5,200 light years distant from your position on the Earth. Look toward the north of two 9th magnitude stars, near the center of NGC 129, and you’ll find the Cepheid variable DL Cassiopeiae. DL Cassiopeiae will fluctuate between 8.6 and 9.3 magnitudes, over the course of an eight-day cycle.
The central star in Cassiopeia’s characteristic W is Gamma Cassiopeiae, a prototype for a class of irregular variable stars believed to be rapidly spinning type-B celestial bodies often fluctuating by as much as magnitude 1.5 or more, Gamma Cassiopeiae will flicker between 2.2 and 3.4 magnitudes as you watch her nightly dance and this star at maximum brightness outshines both Alpha Cassiopeiae and Beta Cassiopeiae. Astronomers believe these apparent fluctuations are due to a decretion disk around this star resulting from the rapid spinning of the star, which results in some of the star’s mass forming a decretion disk. Gamma Cassiopeiae is also a spectroscopic binary star with an orbital period of about 204 days and astronomers believe Gamma Cassiopeiae’s companion star is about the same relative mass as Sol. Part of a small group of stellar sources in the night sky that beam X-ray radiation about 10 times higher than the X-rays emitted from other type-B stars across the cosmos, Gamma Cassiopeiae exhibits both short-term and long-term cycles of x-ray emission. Stargazers should also be able to view Gamma Cassiopeiae as an optical double star, with a faint magnitude 11 companion star, about 2 arcseconds distant from Gamma Cassiopeiae.
Chinese astronomers studied Gamma Cassiopeiae
Ancient stargazers in China called Gamma Cassiopeiae Tsih, which loosely translates as “the whip”, but no references have been found in Arabic or Latin texts of Gamma Cassiopeiae being referred to using a different name. Modern stargazers refer to Gamma Cassiopeiae by a number of different designations, including 27 Cassiopeiae, HR 264, HD 5394, and others. Modern astronauts often use Gamma Cassiopeiae as a star guide because it’s a relatively bright celestial object and in previous space missions this star was used as an easily recognizable navigational reference point in the night sky.
Astronomers note two Messier objects
M103 (NGC 581) is the first of two Messier objects in Cassiopeia’s arms viewable through a six-inch time-machine-to-the-stars and should appear as about three dozen stars grouped in a triangular area 6′ across. A fairly compact open cluster, M103 will be 1 degree east of Delta Cassiopeiae, and is the left bottom star of Cassiopeia’s characteristic W shape marking her throne in the night sky. Pierre Mechain was first given credit for seeing this open cluster in the night sky in 1781. Stargazers using 8×50 binoculars will see about 25 magnitude 10 or fainter stars in their view and a string of four stars immediately to M103’s southeast, which adds to the beauty of viewing M103, significantly.
The second Messier object in Cassiopeia cataloged by Messier is M52 (NGC 7654), you can locate M52 by drawing a line from Alpha Cassiopeiae through Beta Cassiopeiae, and then extending your line an equal distance to M52. An 8-inch time-machine-to-the-stars will reveal about 75 stars in the night sky clumped in various patterns along the edge of the Milky Way that aren’t lost among the background points of light behind these stars. One of the richest open clusters in Cassiopeia’s arms and north of the celestial equator, Messier made note of M52 in his catalog in 1774. This open cluster will appear as a nebulous mass of about 100 stars in 8×50 astronomical binoculars, with a few individual stars that you can resolve a little better. Stargazers looking for a little extra should look to the north of M52 to find Harrington 12, a wide triangular looking asterism containing about a dozen 5th to 9th magnitude stars, which will appear spectacular in low-power astronomical binoculars.
The Owl spreads its wings
Journey less than 3 degrees south of Delta Cassiopeiae to find the spectacular Owl Cluster (NGC 457), a celestial object ancient stargazers could plainly see in the north night sky, the Owl Cluster’s wings will be clearly viewable using a 4-inch time-machine-to-the-stars. Stargazers can also locate Delta Cassiopeiae by using 5th magnitude Phi Cassiopeiae and 7th magnitude HD 7902, which lie to the southeast of the Owl Cluster. The Own’s eastern wing is a line of four bright stars while the western wing is composed of two pairs of stars arranged in a long rectangle. The brightest star in the Owl Cluster will shine at 8.6 magnitude and will appear a little orange in color to star gazers.
Deep Impact approaches comet Hartley 2 and will arrive at its nearest location on November 4
Astronomy News – NASA’s EPOXI mission is currently on a journey to comet Hartley 2 and Deep Impact as this mission is more commonly referred too will arrive at its nearest spot to this icy world on November 4. NASA was using imagers on Deep Impact during the days between September 9-17 to get a view of comet Hartley 2 before the spacecraft arrives on location and the things they saw has NASA’s comet scientists shaking their heads. Apparently, comet scientists observed the characteristic increase in the release of cyanide associated with comets as they travel through the inner solar system, by a factor of five or six times during this observation period in September. What they didn’t see was the expected increase in dust emissions due to this fivefold increase in the release of cyanide, which is something new according to comet scientists, who are now busy trying to figure out what they actually saw.
Comets could hold the keys to understanding the beginnings of life on Earth
Why would the difference be so important to comet scientists as Deep Impact approaches comet Hartley 2? Scientists hate unknown parameters being suddenly thrown into their well-calculated plans and this discovery certainly could affect the mission in ways we’ll possibly never hear about. Where did the dust go? The dust obviously didn’t go anywhere and is still close to comet Hartley 2, which could affect the quality of the view observers will get of Hartley 2. This will especially be true for observers on Earth, who now that they know about this fact can certainly take this fact into consideration. Otherwise, this fact is going to skew your observations and your interpretation of what you’re actually seeing when trying to view comet Hartley 2 from Earth. Certainly, this isn’t likely to seriously affect the mission as a whole, and Deep Impact will surely get some spectacular pictures of comet Hartley 2 as it approaches and recedes from the sun.
We’ll never know if we don’t go out there and study them
The interesting thing about comets releasing significant amounts of cyanide is that cyanide is a carbon-based molecule that certainly could have been brought to Earth on comets like Hartley 2 billions of years in the past. Comets haven’t changed since this time and have been hitting the Earth and releasing cyanide since this time, which brings up interesting questions that NASA is hoping the EPOXI mission and follow up missions to other comets is going to answer in the years ahead.