Brett Joseph captured Venus in the east, very near the sunrise point, on October 31, 2018, less than a week after the planet passed between us and the sun and thereby entered the morning sky. Why could he see Venus so near the sunrise? Because Venus is very bright!
Jupiter is a bright planet, and Mars was also exceedingly bright for a couple of months, centered on late July, 2018. But neither Jupiter nor Mars at its brightest can outshine Venus.
Our neighboring world – orbiting one step inward from Earth around the sun – is the third-brightest object in the sky, after the sun and moon. In late November and early December, 2018, Venus is easily visible in the east before sunup. It’s at its brightest around this time for this entire morning apparition, which extends into 2019.
Why is this world so bright?
Larry Estes in North Richland Hills, Texas caught this image of Venus with a Samsung Galaxy S9 phone on November 13, 2018. He wrote: “Went out for star shots and Venus was so bright that I thought it was a plane coming, at first. When sunrise came it took this shot from the top of my car. Could lie and say it was a calm body of water, but it is the reflection onto the top of my car.”
As the planet next-inward from Earth in orbit around the sun, Venus is relatively nearby. But its nearness isn’t the only reason Venus is bright. Consider that Mars orbits one step outward from Earth. And Mars waxes and wanes in brightness in our sky. It’s only exceptionally bright around the time Earth passes between Mars and the sun, when the Red Planet is at its closest to us, which it was earlier this year, around late July.
With Venus, something else is going on. Astronomers use the term albedo to describe how bright a planet is in absolute terms. When sunlight strikes a planet, some of the light is absorbed by the planet’s surface or atmosphere – and some is reflected. Albedo is a comparison between how much light strikes an object – and how much is reflected.
As you might have guessed, Venus has the highest albedo of any major planet in our solar system.
Throughout November of 2018, Venus has been near a bright star, Spica in the constellation Virgo. Spica is one of the brightest stars in our sky but it’s nowhere near as bright as Venus! A. Kannan caught Venus and Spica on November 13, 2018 and wrote: “The planet Venus and Star Spica shines brightly at dawn before sunrise in Singapore. The pair looks so beautiful in the dark sky.”
The albedo of Venus is close to .7, meaning it reflects about 70 percent of the sunlight striking it. When the moon is close to full in Earth’s sky, it can look a lot brighter than Venus, but the moon reflects only about 10 percent of the light that hits it. The moon’s low albedo is due to the fact that our companion world is made of dark volcanic rock. It appears bright to us only because of its nearness to Earth. It’s only about a light-second away, in contrast for several light-minutes for Venus.
Venus is bright (it has a high albedo) because it’s blanketed by highly reflective clouds. The clouds in the atmosphere of Venus contain droplets of sulfuric acid, as well as acidic crystals suspended in a mixture of gases. Light bounces easily off the smooth surfaces of these spheres and crystals. Sunlight bouncing from these clouds is a big part of the reason that Venus is so bright.
By the way, Venus isn’t the most reflective body in our solar system. That honor goes to Enceladus, a moon of Saturn. Its icy surface reflects some 90% of the sunlight striking it.
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Since Venus passed between us and the sun in late October, 2018, its lighted half – or day side – is still facing mostly away. It’s an interesting fact that this crescent Venus can appear brighter than the fuller Venus we see at other times. Read more about why. This crescent Venus was captured by Prabhakaran A on Novermber 20, 2018, from Mleiha, UAE. Equipment: Edge HD 11″ Alt Az – Explore Scientific 3x Extender – ZWO 290MC. Postprocessing: stacked 9000 frames in AS!3 and processed in Registax.
We mentioned above that Mars is brightest when Earth passes between the Red Planet and the sun. At such times, Mars is closest to us, and so it appears brightest in our sky. A similar situation occurs for Venus: the planet is brightest in our sky around the time Venus passes between us and the sun, although not exactly at that time.
Because Venus orbits the sun inside Earth’s orbit, when it goes between us and the sun its lighted hemisphere, or day side, is facing away from us. At such times, it’s difficult or impossible to see Venus at all.
Because it’s an inner planet, as Venus approaches its time of passing between the Earth and sun, we see the planet exhibit phases, like a tiny moon. As Venus draws up behind Earth in orbit – and prepares to “lap” us in the race of the planets – observers on Earth can watch as the phase of Venus wanes. Meanwhile, as the crescent Venus in waning in phase, the overall size of the disk of Venus gets larger in Earth’s sky, as Venus draws closer to us and prepares to go between us and the sun.
Venus is brightest when those two factors combine – waning crescent, plus largest overall size of Venus’ disk – so that the greatest amount of surface area of Venus shows in our sky. Astronomers call this greatest illuminated extent.
In 2018, Venus reached greatest illuminated extent in the evening sky on September 21. It’ll reach greatest illuminated extent in the morning sky on December 1 or 2, 2018, depending on your time zone.
Venus is brightest at what’s called greatest illuminated extent, or greatest brilliancy. It happens when Venus is relatively near Earth, and when telescopes show it in a crescent phase, like a tiny crescent moon. At such times, you can see Venus in the daytime. Read more about how. Here’s a telescopic view of a crescent Venus (l) and the moon, in daytime, via NASA.
Bottom line: Venus is the third-brightest object in the sky, after the sun and moon. That’s partly because sunlight is easily reflected by acidic clouds in the atmosphere of Venus.
from EarthSky https://ift.tt/2FI7d5P
Brett Joseph captured Venus in the east, very near the sunrise point, on October 31, 2018, less than a week after the planet passed between us and the sun and thereby entered the morning sky. Why could he see Venus so near the sunrise? Because Venus is very bright!
Jupiter is a bright planet, and Mars was also exceedingly bright for a couple of months, centered on late July, 2018. But neither Jupiter nor Mars at its brightest can outshine Venus.
Our neighboring world – orbiting one step inward from Earth around the sun – is the third-brightest object in the sky, after the sun and moon. In late November and early December, 2018, Venus is easily visible in the east before sunup. It’s at its brightest around this time for this entire morning apparition, which extends into 2019.
Why is this world so bright?
Larry Estes in North Richland Hills, Texas caught this image of Venus with a Samsung Galaxy S9 phone on November 13, 2018. He wrote: “Went out for star shots and Venus was so bright that I thought it was a plane coming, at first. When sunrise came it took this shot from the top of my car. Could lie and say it was a calm body of water, but it is the reflection onto the top of my car.”
As the planet next-inward from Earth in orbit around the sun, Venus is relatively nearby. But its nearness isn’t the only reason Venus is bright. Consider that Mars orbits one step outward from Earth. And Mars waxes and wanes in brightness in our sky. It’s only exceptionally bright around the time Earth passes between Mars and the sun, when the Red Planet is at its closest to us, which it was earlier this year, around late July.
With Venus, something else is going on. Astronomers use the term albedo to describe how bright a planet is in absolute terms. When sunlight strikes a planet, some of the light is absorbed by the planet’s surface or atmosphere – and some is reflected. Albedo is a comparison between how much light strikes an object – and how much is reflected.
As you might have guessed, Venus has the highest albedo of any major planet in our solar system.
Throughout November of 2018, Venus has been near a bright star, Spica in the constellation Virgo. Spica is one of the brightest stars in our sky but it’s nowhere near as bright as Venus! A. Kannan caught Venus and Spica on November 13, 2018 and wrote: “The planet Venus and Star Spica shines brightly at dawn before sunrise in Singapore. The pair looks so beautiful in the dark sky.”
The albedo of Venus is close to .7, meaning it reflects about 70 percent of the sunlight striking it. When the moon is close to full in Earth’s sky, it can look a lot brighter than Venus, but the moon reflects only about 10 percent of the light that hits it. The moon’s low albedo is due to the fact that our companion world is made of dark volcanic rock. It appears bright to us only because of its nearness to Earth. It’s only about a light-second away, in contrast for several light-minutes for Venus.
Venus is bright (it has a high albedo) because it’s blanketed by highly reflective clouds. The clouds in the atmosphere of Venus contain droplets of sulfuric acid, as well as acidic crystals suspended in a mixture of gases. Light bounces easily off the smooth surfaces of these spheres and crystals. Sunlight bouncing from these clouds is a big part of the reason that Venus is so bright.
By the way, Venus isn’t the most reflective body in our solar system. That honor goes to Enceladus, a moon of Saturn. Its icy surface reflects some 90% of the sunlight striking it.
Enjoying EarthSky so far? Sign up for our free daily newsletter today!
Since Venus passed between us and the sun in late October, 2018, its lighted half – or day side – is still facing mostly away. It’s an interesting fact that this crescent Venus can appear brighter than the fuller Venus we see at other times. Read more about why. This crescent Venus was captured by Prabhakaran A on Novermber 20, 2018, from Mleiha, UAE. Equipment: Edge HD 11″ Alt Az – Explore Scientific 3x Extender – ZWO 290MC. Postprocessing: stacked 9000 frames in AS!3 and processed in Registax.
We mentioned above that Mars is brightest when Earth passes between the Red Planet and the sun. At such times, Mars is closest to us, and so it appears brightest in our sky. A similar situation occurs for Venus: the planet is brightest in our sky around the time Venus passes between us and the sun, although not exactly at that time.
Because Venus orbits the sun inside Earth’s orbit, when it goes between us and the sun its lighted hemisphere, or day side, is facing away from us. At such times, it’s difficult or impossible to see Venus at all.
Because it’s an inner planet, as Venus approaches its time of passing between the Earth and sun, we see the planet exhibit phases, like a tiny moon. As Venus draws up behind Earth in orbit – and prepares to “lap” us in the race of the planets – observers on Earth can watch as the phase of Venus wanes. Meanwhile, as the crescent Venus in waning in phase, the overall size of the disk of Venus gets larger in Earth’s sky, as Venus draws closer to us and prepares to go between us and the sun.
Venus is brightest when those two factors combine – waning crescent, plus largest overall size of Venus’ disk – so that the greatest amount of surface area of Venus shows in our sky. Astronomers call this greatest illuminated extent.
In 2018, Venus reached greatest illuminated extent in the evening sky on September 21. It’ll reach greatest illuminated extent in the morning sky on December 1 or 2, 2018, depending on your time zone.
Venus is brightest at what’s called greatest illuminated extent, or greatest brilliancy. It happens when Venus is relatively near Earth, and when telescopes show it in a crescent phase, like a tiny crescent moon. At such times, you can see Venus in the daytime. Read more about how. Here’s a telescopic view of a crescent Venus (l) and the moon, in daytime, via NASA.
Bottom line: Venus is the third-brightest object in the sky, after the sun and moon. That’s partly because sunlight is easily reflected by acidic clouds in the atmosphere of Venus.
from EarthSky https://ift.tt/2FI7d5P
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