How Far is Mercury from Earth?

Orbit of Mercury

Although Galileo wasn’t able to see the phases of Mercury (like the phases of Venus and the Moon) with his first crude telescope, the astronomers that carried on his discoveries did. This was powerful evidence that both Mercury and Earth are orbiting the Sun.

You can also check out these amazing books for more information about the planet Mercury.

Since Mercury orbits the Sun, and it follows a very elliptical path on its journey around the Sun, our two planets can vary their distance significantly.

When Mercury is at its closest point to Earth, astronomers call this opposition (from the point of view of Mercury). This would happen when Mercury was at its furthest from the Sun, and Earth is at its closest. When this happens, Mercury and Earth would be separated by only 77 million km (48 million miles).

Their maximum distance occur when Earth is at its furthest point from the Sun, and Mercury is at its maximum on the other side of the Sun. The three objects then line up perfectly. At this point, Mercury and Earth can be 222 million km (138 million miles) apart.

Distancia desde la Tierra a Mercurio

How Far is Venus from Earth?

The are varying numbers for the Venus distance from Earth. Each number depends on the relative position of each planet in its elliptical orbit. The point when the planets are at their closest approach to each other is called opposition. The distance between the planets can even vary at different oppositions. The closest possible opposition distance between Earth and Venus is 38 million kilometers. This is the closest that any planet comes to Earth.

The farthest that Venus ever gets from Earth is 261 million km. The means that the Venus distance from Earth can vary by an incredible 223 million km. While that seems like an amazing distance, it is nothing compared to the numbers attributed to other planets. Try to imagine how far it is between Earth and Neptune. Here is a link that tells you how to figure those distances out.

The relative proximity of Venus helps to explain why it is the second brightest object in the night sky. The planet has an apparent magnitude of about -4.9 at its brightest. It can also completely disappear from the night sky when it is at its most distant, because the Sun is between it and the Earth. The planet’s apparent magnitude is also helped by the reflectivity of the sulfuric acid clouds that dominate its atmosphere. The clouds reflect a great deal of visible light, increasing the planet’s albedo and making it more readily seen.

Venus will periodically pass across the face of the sun. This is called a transit. These transits of Venus occur in pairs with more than a century separating each pair. Since the advent of the telescope, transits have been observed in 1631, 1639; 1761, 1769; and 1874, 1882. the most recent occurred on June 8, 2004. The second in this pair will occur on June 6, 2012, so mark your calenders and prepare your telescopes. The planet can also be seen to go through phases much like the Moon when you observe it through powerful binoculars or small telescopes.

Venus is always brighter than any star. It is at its brightest when the Venus distance from Earth is the smallest. The planet can be easy to see when the Sun is low on the horizon, it always lies about 47° from the Sun. The planet orbits faster than the Earth, so overtakes it every 584 days. When this happens Venus is more easily seen in the morning, just after sunrise. Hopefully, you have found quite a bit of useful information here.

We have written many articles about Venus for Universe Today. Here are some interesting facts about Venus, and here’s an article about Venus compared to Earth.

If you’d like more information on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide on Venus.

We’ve also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.

References:
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Venus&Display=OverviewLong
http://curious.astro.cornell.edu/question.php?number=564

Astronomy Day – May 10, 2008

Are you ready for Astronomy Day? Astronomy Day is a grass roots movement designed to share the joy of astronomy with the general population – “Bringing Astronomy to the People.” During this year’s Astronomy Day on May 10, thousands of people who have never looked through a telescope will have an opportunity to see first hand what has so many amateur and professional astronomers all excited!

Astronomy clubs, science museums, observatories, universities, planetariums, laboratories, libraries, and nature centers host special events and activities to acquaint their population with local astronomical resources and facilities. Many of these events are located at non-astronomical sites; shopping malls, parks, urban centers – truly Bringing Astronomy to the People. If you’re interested in attending such an event, take a look at where current Astronomy Day events being held. This list only encompasses those groups who choose to advertise on the Astronomical League website, so please be sure to check your local news media for other events.

If you, your facility, group or astronomy club is interested in planning astronomy day activities, perhaps you’d like some help! By following the link to the Sky and Telescope Astronomy Day Handbook you can get some great pointers and ideas by downloading the free handbook written by David Levy. While on the page, be sure to visit other great links such as Let’s Go Stargazing and downloadable handouts like the Good Neighbor Outdoor Lighting flyer. The Astronomical League also offers Graphics For Astronomy Day Events and you can even enter your activities in the annual Sky and Telescope Astronomy Award Program!

Need more fun things to do for Astronomy Day that you can reach with just a mouse click? Then know the Abrams Sky Calendar is available for Astronomy Day activities. Anyone celebrating the event is welcome to distribute any number of copies of the Sky Calendar or Sample Sky Map with no restrictions, other than we ask that material not be deleted. How about kid’s activities? Let’s start with coloring pages for Jupiter, Saturn and Mars. You can even make your own Solar System Mobile!

Astronomy Day is an astronomical public relations event that helps highlight ways the general public can get involved with astronomy – or at least get some of their questions about astronomy answered. This important event – Astronomy Day – is co-sponsored by 14 astronomical and astronomy education organizations. They are: The Astronomical League, The Astronomical Society of the Pacific, the Royal Astronomical Society of Canada, the American Astronomical Society, the Astronomical Association of Northern California, the Western Amateur Astronomers, the American Association of Physics Teachers, the Association of Lunar and Planetary Observers, the American Meteor Society, the American Association of Variable Star Observers, the Planetary Society, the National Space Society, the International Planetarium Society, the Association of Astronomy Educators, and the International Astronomical Union.

As the Executive Secretary of the Astronomical League, I’m here to answer any Astronomy Day questions you might have – or point you in the right direction. Spend a few minutes coloring with a child, set up your telescope for a neighbor, take binoculars to work, make copies of the Sky Calendar and Maps and post in your local library. No matter what the size or your event, or level of involvement, it’s all about sharing what you love to do with others. Celebrate Astronomy Day!

Atmosphere of Venus



Earth and Venus share many physical characteristics. Atmosphere is not one of them. The atmosphere of Venus is so harsh that it is the main reason that no one has ever been able to make optical observations of anything other than the planet’s upper atmosphere.

Visualization of the planet is made impossible be the high amounts of sulfuric acid in the atmosphere. Clouds in the upper atmosphere are full of sulfuric acid droplets. Sulfur is highly reflective of visible light, thus preventing observation much deeper than the upper limits of the clouds themselves.

The next challenge that the atmosphere of Venus presents is its composition. It is made up of 96% carbon dioxide. Oxygen can not be detected even as a trace element. At the surface the atmospheric pressure is 92 times that of Earth. If you were able to find a way to survive the intense pressure and had enough oxygen, you would be standing on a surface that is hot enough to melt lead. The temperature across Venus, from pole to pole, is a steady 462°C as a result of the atmosphere’s greenhouse qualities. In the hottest parts of the hottest deserts here on Earth, the temperatures never top 50°C.

The sweltering surface of the planet is covered by volcanoes, impact craters, and old lava flows. There are 1,000 volcanic craters and crater remnants that are over 20 km in diameter. The surface has never been impacted by a small meteorite. The atmosphere burns up anything small. It could take an asteroid in excess of 50 km to survive long enough to hit the surface and then it would have lost close to half of its mass in the atmosphere. The entire planet was resurfaced by volcanic flows between 300 and 500 million years ago.

Several spacecraft have entered the atmosphere of Venus. The first successful probe was the Soviet mission Venera 3, but its instruments failed before entry. Venera 4successfully deployed a number of science experiments. They showed a surface temperature of almost 500°C and an atmosphere that was 90 to 95% carbon dioxide. The atmosphere was much denser than anticipated and its slower descent caused its batteries to run down before reaching the surface. NASA’s Mariner 5 reached the planet one day after Venera 4, but only flew by. The data from the two missions were compared and were an early step in international space exploration cooperation. The Soviet space agency also launched Venera’s 5 and 6. They returned a great deal of information, but were crushed by atmospheric pressure within 20 km of the surface.

There have been over a dozen missions to study the surface and atmosphere of Venus since the Venera program. Currently, the Venus Express mission is in orbit. Bepicolumbo and the Venus in-Situ Explorer are planned. Each mission returns new data, it is hard to imagine what mysteries may be unraveled with a surface explorer.

We have written many articles about Venus for Universe Today. Here are some interesting facts about Venus, and here are some pictures of planet Venus.

If you’d like more information on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide on Venus.

We’ve also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.

References:
http://www.nasa.gov/audience/forstudents/5-8/features/F_The_Planet_Venus_5-8.html
http://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.html
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Venus&Display=OverviewLong

History of Planet Venus



Venus is one of the 5 planets visible to the unaided eye, and so it has been seen in the sky since prehistoric times. After the Sun and the Moon, Venus is the brightest object in the sky – brighter than any stars.

Venus is the Roman name for the Greek goddess of love; Aphrodite. But there are references to Venus as far back as Babylonian cuneiformic texts, like the Venus table of Ammisaduqa which could be as old as 1600 BC. Ancient Egyptians thought that Venus was actually two separate objects… a morning star, and then a completely different evening star. The tradition carried on with the ancient Greeks, as well.

The early mathematician Pythagoras was one of the first to recognize that the morning and evening stars were actually the same object: Venus. So perhaps he was the first to “discover Venus”.

The Maya civilization held Venus in high regard, and the planet figured prominently in their religious calendar.

Once he built his first rudimentary telescope, Galileo turned it towards Venus, was was astonished to find that the planet goes through phases like the Moon, going from crescent to gibbous to full and then back again. This was one of the strongest pieces of evidence that Venus goes around the Sun, and not the Earth as others originally believed.

Because Venus has always been obscured by thick clouds, science fiction writers have been free to imagine whatever they wanted existed on the surface of Venus. The clouds helped them to imagine a warm tropical world with constant rainfall and lush vegetation. The truth, of course, is that Venus is a hellish hot world, devoid of life.

Spock’s Astronomy Quiz

Leonard Nimoy as Mr. Spock. Credit: CBS Television

Have you ever wanted to test your astronomy knowledge against the best? Then take the warp speed jump to Spock’s Astro Quiz. It’s more than just astronomy trivia, it’s a great way to test your astronomy knowledge, learn more about astronomy related topics and interact via live chat with others interested in astronomy…

Welcome to Spock’s Astro Quiz, a great place to see just how much you know about astronomy and to enjoy the company of astronomy minded individuals. No special knowledge, secret passwords, or fancy hoops to jump through to enjoy the fun… All you have to do is click Log In and get started!

While you’re there, this interactive site will not only allow to test your astronomy skill against Spock’s, but to chat live with astronomy-minded visitors and play against each other as well. Just a word of caution though… Spock plays a clean astronomy game. Use a swear word and you’ll be warned once. Do it again and you’re permanently beamed out. The astronomy quiz and astronomy chat board is continually monitored and safe for players of all ages. Solicitors of any type will be immediately banned.

Test your astronomy skill… Enjoy the company of other astronomy friends during cloudy nights… And live long and prosper!

Brought to you by Macedon Ranges Observatory.

Pictures of Planet Venus

Venus is one of the brightest objects in the night sky, so it’s not surprising that it’s been photographed many times. Some pictures of Venus have been taken from here on Earth, while other Venus pics have been taken from spacecraft orbiting the planet. You might be surprised to know that spacecraft have even landed on Venus (they didn’t last long), and took images of Venus from the surface.

Surface Image of Venus
This is a picture of Venus captured by NASA’s Magellan spacecraft. It shows the entire surface of the planet, imaged by the spacecraft’s radar instrument, which can penetrate the thick clouds to reveal the surface below. Magellan was launched from the cargo bay of the space shuttle Atlantis in May 1989, and arrived at Venus on August 10, 1990. It orbited the planet for 4 years before plunging to the surface.


3-D Image of Venus’ Surface
This is another photograph of Venus taken by NASA’s Magellan spacecraft. Planetary scientists used the radar data captured by Magellan to build up 3-dimensional images of the planet’s surface. This is an image of the Eistla Regio region, which contains volcanos and impact craters.



Photo of Venus from Pioneer Venus Spacecraft
This was one of the first ever close-up photographs of Venus, captured by NASA’s Pioneer Venus spacecraft. It’s actually a false color image made from ultraviolet images of the planet Venus by the spacecraft. The Pioneer Venus Orbiter went into orbit around Venus on December 4, 1978, and released several probes into Venus’ atmosphere to study it.


The Surface of Venus by Venera
You might be amazed to know that spacecraft have actually landed on the surface of Venus and sent pictures back. The Soviets sent a fleet of Venera spacecraft to Venus, and several actually made it down to the surface. Here’s a color photograph of Venus captured by the Venera 13 spacecraft, which landed on the surface of Venus on March 3, 1982.



Picture of Venus by Venus Express
This is a false-color image of Venus taken by the Venus Monitoring Camera on board ESA’s Venus Express spacecraft. It’s showing the planet’s southern hemisphere, including its south pole. The spacecraft captured the image when it was 35,000 km from the surface of Venus.

Photos of the Earth and Moon – From Other Worlds

Image taken by the HiRISE camera on NASA's Mars Reconnaissance Orbiter, showing Earth and the Moon. Credit: NASA/JPL

We’re familiar with the close-up images of Earth captured by orbital satellites and astronauts on the International Space Station. But here are a few pictures of the Earth and Moon captured at a distance, while passing around the Moon, or orbiting distant Saturn. In the words of Carl Sagan, “Look again at that dot. That’s here. That’s home. That’s us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives.”

Since Sagan commented on Voyager 1’s image of Earth, several more pics of the Earth and Moon have been captured that really put our tiny spot in the Universe into perspective.


Voyager 1 – the Pale Blue Dot
This image, captured by NASA’s Voyager 1 spacecraft on February 14, 1990, is the one Sagan was talking about. It was taken when Voyager 1 was about 6.4 billion kilometres (4 billion miles) from Earth. In this image, the entirety of the planet takes up less than a single pixel; in fact, NASA calculated that we’re only 0.12 pixel in size. Sagan pushed the agency to capture images of all the planets in the Solar System, to create a family portrait seen from Voyager’s distant position.



Cassini – the Earth from Saturn
This is easily the best picture ever captured by NASA’s Cassini spacecraft, and in the running for the best space pictures of all time. It shows Saturn in all its glory, backlit by the Sun. From this view, the rings glow with an ethereal light.

But this image is extra special. Take a look towards the upper left of the image, and you’ll notice a tiny blue-white dot. Once again, there’s Earth, seen from a distance of 1.4 billion km (1 billion miles).


Mars Express – the Earth and Moon from Mars
ESA’s Mars Express captured this image of Earth and the Moon on July 3, 2005 when it was 8 million km (5 million miles). This was actually the first observational data sent back by the probe. A fitting introduction to Martian system. Of course, Mars Express was designed to image the relatively nearby surface of Mars, and not such distant objects, so the resolution of the image isn’t very good. And yet, they’re instantly recognizable as the Earth and Moon.

Opportunity Rover – the Earth from the Surface of Mars

Here’s an image of Earth captured from the surface of another planet. In this case, we’re seeing Earth from Mars, as photographed by NASA’s Mars rover Opportunity on April 29, 2005. Normally operating only in the Martian day, Opportunity woke up a little after sunset, and captured this image of Earth as the stars were starting to come out. The image of Earth looks a little elongated because it was moving slightly during the 15-second exposures. Imagine what some future Martian might see, stepping out onto the surface of the Red Planet in the dusky twilight to see our bright planet in the sky.


Rosetta – Earth and Moon during a flyby

Now this is what you might have been expecting to see. A picture of Earth, with the continents clearly visible. This photograph of Earth and the other of the Moon were taken by ESA’s Rosetta spacecraft during a flyby on November 15, 2007. Rosetta’s primary mission is to visit Comet 67P/Churyumov-Gerasimenko in May 2014, but this flyby was a great opportunity for Rosetta to test out its OSIRIS camera system. The image of the Moon was taken separately.


Earthrise – seen from the Moon
This is the classic “Earthrise” photograph, captured by astronaut William Anders during the historic Apollo 8 mission – the first human mission to the Moon. This photograph was taken on December 24, 1968. If you’re standing on the surface of the Moon, the Earth doesn’t actually “rise”. Since the Moon is tidally locked to the Earth, our planet always hangs in exactly the same point of the sky. It takes an orbiting spacecraft to see the Earth actually rise from the horizon.

This photograph was recreated by the Japanese Kaguya spacecraft, which captured a similar sequence of the Earth using its high-definition video camera.

Earth from Galileo
And finally, I think I’ve saved one of the best pictures for last. This is a photograph of the Earth and Moon (not to scale) captured by NASA’s Galileo spacecraft as it was speeding away towards Jupiter. Galileo captured these images in 1992, and finally reached the Jovian system in 1995-97. You’re looking at the Pacific Image, with South America visible as well as the Caribbean.

XMM-Newton Discovers Part of Missing Matter in the Universe

We’re getting the numbers down pretty well now about how much we don’t know about the universe: Only about 5% of our universe consists of normal matter, made of atoms. The rest of our universe is composed of elusive matter that we don’t understand: dark matter (23%) and dark energy (72%). And of that 5% of normal matter, well, we don’t know what half of that is, either. All the stars, galaxies and gas observable in the universe account for less than a half of all the matter that should be around.

About 10 years ago, scientists predicted that the missing half of ‘ordinary’ or normal matter exists in the form of low-density gas, filling vast spaces between galaxies. The European Space Agency announced today that the orbiting X-ray observatory XMM-Newton has uncovered this low density, but high temperature gas.

The universe has been described as a cosmic web. The dense part of the web is made of clusters of galaxies, which are the largest objects in the universe. Astronomers suspected that low-density gas filled in the filaments of the web. But the low density of the gas has made it difficult to detect. With the XMM-Newton’s high sensitivity, astronomers have discovered the hottest parts of this gas.

Astronomers using XMM-Newton were observing a pair of galaxy clusters, Abell 222 and Abell 223, located 230 million light-years from Earth, when the images and spectra of the system revealed a bridge of hot gas connecting the clusters.

“The hot gas that we see in this bridge or filament is probably the hottest and densest part of the diffuse gas in the cosmic web, believed to constitute about half the baryonic matter in the universe,” says Norbert Werner from SRON Netherlands Institute for Space Research, leader of the team reporting the discovery.

The discovery of this hot gas will help better understand the evolution of the cosmic web.

“This is only the beginning,” said Werner. “To understand the distribution of the matter within the cosmic web, we have to see more systems like this one. And ultimately launch a dedicated space observatory to observe the cosmic web with a much higher sensitivity than possible with current missions. Our result allows to set up reliable requirements for those new missions.”

Original News Source: ESA Press Release

IC 2944 – Astrophotography by Ken Crawford

Do you think you’re seeing a Hubble Image? Then think again. Just revealed at last weekend’s NEAF gathering at Rockland College in Suffern, New York, this incredible image of IC 2944 was taken by Ken Crawford at Macedon Ranges Observatory and shows so much more than just pretty sky scenery. In this edition of the Universe Today Astronomy Photo of the week, we’ll take a deeper look into the science behind the picture as you discover an anomaly known as “Thackeray’s Globules”…

The photographic artistry of Ken Crawford takes us on a visual journey ever deeper into the busy star-forming region, IC 2944. While the view of this incredible emission nebula is some 6,000 light years away, Ken’s work takes us directly in for close up views of Thackeray’s Globules in ways that stagger the imagination.

IC 2948 is sprawling cloud of gas and dust that is illuminated and heated by a loose cluster of massive stars known as IC 2944. These stars are much hotter and much more massive than our Sun and their strong stellar winds carve out unique shapes in the noble hydrogen gases. These busy star forming HII regions are home to curious dark masses which we really don’t know a whole lot about – except their association. Dark globules like these have been known since Dutch-American astronomer Bart Jan Bok first began documenting them in 1947 and astronomer A.D. Thackeray first spied the globules in IC 2944 in 1950.

The largest of the globules in IC 2944 could possibly be two separate clouds that appear to partially overlap along our line of sight. Each cloud is nearly 1.4 light-years along its longest dimension and a combination of both clouds contain enough material to equal over 15 solar masses. When you take a closer look, you’ll see the globules appear almost shattered – as if strong forces were pulling them apart. In the case of IC 2944, seeing is believing because when radio astronomers observed the faint hiss of molecules within the globules, they realized Thackeray’s million year old discovery is in constant, aggressive motion, moving along in a supersonic dance. Like a water droplet sprayed against hot metal, this dance may be caused by the powerful ultraviolet radiation from the luminous, massive stars. When the region of glowing hydrogen gas is heated, it expands and streams against these dark masses, causing their annihilation.

According the research done by Bo Reipurth, Patrice Corporon, Michael Olberg and Guillermo Tenorio-Tagle: “We believe that the globules are the remnants of an elephant-trunk observed from behind, originating as a Rayleigh-Taylor instability in an expanding neutral shell powered by the hot HII region. The globule complex is now in an advanced stage of disintegration. We have found no evidence for star formation in any of the globules.”

Often known as the Running Chicken Nebula or the Lambda Cen Nebula, IC 2944 and IC 2948 is nestled between the Southern Cross and the star-thick Carina area on the southern border of Centaurus (RA 11:36.6 Dec -63:02). With an average magnitude of 4.5 and spanning around 75 arc minutes, its collection of bright stars is also referred to as Collinder 249 and was given the designation of Caldwell 100 by Sir Patrick Moore. Don’t expect to see a vision in either eyepiece or binoculars. The cluster is easy… But the nebula is very vague!

Image Details: IC 2944
Taken at: MACEDON RANGES OBSERVATORY
AP130 @ F6 / Paramount ME
Apogee Alta 16803
AstroDon – (5nm Ha & SII) & OIII 3nm Filters
Ha =180 minutes mapped to Green
SII =180 minutes Mapped to Red
OIII = 240 minutes Mapped to Blue
CCDAutoPilot for unattended imaging With MaxDL 4