APOD: Mars in the Loop (2012 Aug 09)

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Expand view Topic review: APOD: Mars in the Loop (2012 Aug 09)

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Fri Aug 10, 2012 8:56 pm

Keyman wrote:
Anthony Barreiro wrote:When an outer planet's opposition (or the inferior conjunction of an inner planet) is farther from the ecliptic (farther from a node) you get a loop, and when it's closer to the ecliptic (closer to a node) you get an S-shaped path.
...so that when/if it's AT a node, you'd get the "line" waterfeller was envisioning?
Yes, almost. When an outer planet is at opposition at the same time that it is crossing Earth's ecliptic plane (i.e. at one of its nodes) it will follow an S-shaped path that is so shallow that it will be virtually indistinguishable from a straight line. The same will be true for an inner planet that reaches inferior conjunction at the same time it crosses Earth's ecliptic plane.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Fri Aug 10, 2012 8:32 pm

ta152h0 wrote:Is this the same process the smart ones use to determine if stars have planets orbiting, " the wobble " ?
No. Stars that wobble because of their planets are examined spectroscopically, since the wobble introduces Doppler shift.

Re: APOD: Mars in the Loop (2012 Aug 09)

by ta152h0 » Fri Aug 10, 2012 8:04 pm

Is this the same process the smart ones use to determine if stars have planets orbiting, " the wobble " ?

Re: APOD: Mars in the Loop (2012 Aug 09)

by kilocharliemike » Fri Aug 10, 2012 5:12 pm

What an amazing series! And thanks for the one sentence explanation of retrograde motion, very helpful!

Re: APOD: Mars in the Loop (2012 Aug 09)

by Keyman » Fri Aug 10, 2012 2:07 pm

Anthony Barreiro wrote:When an outer planet's opposition (or the inferior conjunction of an inner planet) is farther from the ecliptic (farther from a node) you get a loop, and when it's closer to the ecliptic (closer to a node) you get an S-shaped path.
...so that when/if it's AT a node, you'd get the "line" waterfeller was envisioning?

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Fri Aug 10, 2012 1:26 pm

Anthony Barreiro wrote:We do seem to be talking about different things. Perhaps I misunderstood waterfeller's question. We had started talking about why Mars' path before and after opposition is a loop rather than a straight line. That has to do with Mars' apparent motion north and south relative to Earth's ecliptic plane, i.e. where Mars is relative the nodes. When an outer planet's opposition (or the inferior conjunction of an inner planet) is farther from the ecliptic (farther from a node) you get a loop, and when it's closer to the ecliptic (closer to a node) you get an S-shaped path.
Yes. The question is specifically when the planes intersect, which is better expressed as where the planes intersect. Obviously, two planes intersect in a line (which passes through the Sun). Earth will cross that line twice a year, always on the same dates and almost exactly 6 months apart. Mars will cross the line twice every Mars year, on the same Martian dates, but changing Earth dates. Since the line of intersection isn't along Mars's semimajor orbital axis, the two crossing dates are not evenly spaced in the Martian year (due to Mars's fairly eccentric orbit).

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Fri Aug 10, 2012 6:12 am

Chris Peterson wrote:Right, but we're talking about different things. The nodes define when Mars itself crosses the ecliptic, which happens about once a year (because of Mars's ~2 year orbit) and which depends on the position of Mars- so the Earth date changes. The question, however, was on what dates does the Earth cross the plane of Mars's orbit. That doesn't depend on the position of Mars at all, only the position of the Earth, and because the two planes are fixed (ignoring very long precession cycles), the dates don't change.
We do seem to be talking about different things. Perhaps I misunderstood waterfeller's question. We had started talking about why Mars' path before and after opposition is a loop rather than a straight line. That has to do with Mars' apparent motion north and south relative to Earth's ecliptic plane, i.e. where Mars is relative the nodes. When an outer planet's opposition (or the inferior conjunction of an inner planet) is farther from the ecliptic (farther from a node) you get a loop, and when it's closer to the ecliptic (closer to a node) you get an S-shaped path.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Ann » Fri Aug 10, 2012 3:20 am

Chris Peterson wrote:
Ann wrote:Interestingly, it was the orbit of Mars (as measured by Tycho Brahe) that made Johannes Kepler realize that the planets follow elliptical orbits around the Sun. The orbit of Mars is, incidentally, more elliptical than the orbit of the Earth.
Although your meaning is clear, it would be better to say "more eccentric" than "more elliptical", as eccentricity is the measure of how out-of-round an ellipse is (and even a circle is actually an ellipse).
An eccentric old lady, Madame de Meuron, with an elliptical hat and ear trumpet.



Ann

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Fri Aug 10, 2012 12:25 am

Anthony Barreiro wrote:
Chris Peterson wrote:
waterfeller wrote:Out of curiosity, what is the angle between the two planes and when during our year do they intersect?
Mars is inclined 1.85° to the ecliptic. To calculate the intersection dates, you need to look at the orbital elements for both Earth and Mars, specifically the longitude of the ascending node. Of course, the Earth crosses Mars's orbital plane exactly twice a year; by my calculation around May 10 and November 11. Obviously these crossings are almost exactly 6 months apart, given the very nearly circular orbit of the Earth.
I'm not that good at math. According to http://spider.seds.org/spider/Mars/mars2012.html , here are the nodes during the previous, current, and next apparitions of Mars (ascending node is when Mars passes from south to north of Earth's ecliptic plane, descending node is when Mars passes from north to south of Earth's ecliptic plane):
20 August 2009 ascending
7 September 2010 descending
8 July 2011 ascending
25 July 2012 descending
25 May 2013 ascending
11 June 2014 descending
Right, but we're talking about different things. The nodes define when Mars itself crosses the ecliptic, which happens about once a year (because of Mars's ~2 year orbit) and which depends on the position of Mars- so the Earth date changes. The question, however, was on what dates does the Earth cross the plane of Mars's orbit. That doesn't depend on the position of Mars at all, only the position of the Earth, and because the two planes are fixed (ignoring very long precession cycles), the dates don't change.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Fri Aug 10, 2012 12:05 am

Chris Peterson wrote:
waterfeller wrote:Of course. With the amazing star background, it is easy to forget that the camera was pointed in a different direction for each picture so we are seeing a different part of the Mars plane, making the "up and down" motion understandable.
Regardless of exactly where the imager had his camera aimed, all the images have been registered against the star background, so effectively we are seeing in just one direction over the entire period of time. In fact, it's because the view isn't changing that we see that up and down motion so clearly.
Out of curiosity, what is the angle between the two planes and when during our year do they intersect?
Mars is inclined 1.85° to the ecliptic. To calculate the intersection dates, you need to look at the orbital elements for both Earth and Mars, specifically the longitude of the ascending node. Of course, the Earth crosses Mars's orbital plane exactly twice a year; by my calculation around May 10 and November 11. Obviously these crossings are almost exactly 6 months apart, given the very nearly circular orbit of the Earth.
I'm not that good at math. According to http://spider.seds.org/spider/Mars/mars2012.html , here are the nodes during the previous, current, and next apparitions of Mars (ascending node is when Mars passes from south to north of Earth's ecliptic plane, descending node is when Mars passes from north to south of Earth's ecliptic plane):
20 August 2009 ascending
7 September 2010 descending
8 July 2011 ascending
25 July 2012 descending
25 May 2013 ascending
11 June 2014 descending

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Thu Aug 09, 2012 11:13 pm

waterfeller wrote:Of course. With the amazing star background, it is easy to forget that the camera was pointed in a different direction for each picture so we are seeing a different part of the Mars plane, making the "up and down" motion understandable.
Regardless of exactly where the imager had his camera aimed, all the images have been registered against the star background, so effectively we are seeing in just one direction over the entire period of time. In fact, it's because the view isn't changing that we see that up and down motion so clearly.
Out of curiosity, what is the angle between the two planes and when during our year do they intersect?
Mars is inclined 1.85° to the ecliptic. To calculate the intersection dates, you need to look at the orbital elements for both Earth and Mars, specifically the longitude of the ascending node. Of course, the Earth crosses Mars's orbital plane exactly twice a year; by my calculation around May 10 and November 11. Obviously these crossings are almost exactly 6 months apart, given the very nearly circular orbit of the Earth.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Thu Aug 09, 2012 9:53 pm

waterfeller wrote:
Chris Peterson wrote:
waterfeller wrote:Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...
Mars stays in the same plane, and Earth stays in the same plane... but they are different planes. So our relative "up and down" positions change with respect to each other.
Of course. With the amazing star background, it is easy to forget that the camera was pointed in a different direction for each picture so we are seeing a different part of the Mars plane, making the "up and down" motion understandable. Out of curiosity, what is the angle between the two planes and when during our year do they intersect?
P.S. -- I would defer to an actual astrophotographer on this one, but it seems to me that the camera had to be pointed in the same direction relative to the background stars in order for the stars to appear as points. The composite picture reveals Mars' apparent movement against the background stars.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Thu Aug 09, 2012 9:28 pm

waterfeller wrote:
Chris Peterson wrote:
waterfeller wrote:Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...
Mars stays in the same plane, and Earth stays in the same plane... but they are different planes. So our relative "up and down" positions change with respect to each other.
Of course. With the amazing star background, it is easy to forget that the camera was pointed in a different direction for each picture so we are seeing a different part of the Mars plane, making the "up and down" motion understandable. Out of curiosity, what is the angle between the two planes and when during our year do they intersect?
I poked around a little bit on the internet. The orbital inclination of Mars is only 1.85 degrees relative to the ecliptic, the plane of Earth's orbit around the Sun. (Mercury has the greatest orbital inclination to the ecliptic, 7.01 degrees; Jupiter's is 1.31 degrees.)

The nodes of Mars, i.e. the two points where the plane of the orbit of Mars crosses the plane of the orbit of Earth, occur roughly every Earth year, give or take a month or two from one year to the next. This makes sense, because Mars takes just over two Earth years to complete one orbit around the Sun. I assume the variability arises from the elliptical (eccentric?) shapes of the two planets' orbits and therefore their varying speeds at different distances from the Sun, but that's just a guess. Mars crossed Earth's ecliptic plane from north to south on 25 July 2012, and will cross the ecliptic from south to north on 25 May 2013.

Re: APOD: Mars in the Loop (2012 Aug 09)

by henrystar » Thu Aug 09, 2012 8:50 pm

Ann wrote:
henrystar wrote:I guess that is Leo in the background?
Indeed!

Interestingly, it was the orbit of Mars (as measured by Tycho Brahe) that made Johannes Kepler realize that the planets follow elliptical orbits around the Sun. The orbit of Mars is, incidentally, more elliptical than the orbit of the Earth.

Ann
I finally noticed the rollover, and there indeed was Leo! Lucky Kepler did not try Venus or Mercury: Mars is much more elliptical. But, not THAT elliptical, it was a VERY tough job. And Kepler was nauseated by ellipses, he wanted absolutes of some kind.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Thu Aug 09, 2012 7:16 pm

Anthony Barreiro wrote:
ta152h0 wrote:It would be a perfect haperstance if one of your " unsuspecting passerby"s " was a certain Mr Peterson.
I'm sure I would say something stupid, like "elliptical" rather than "eccentric", and need to be corrected. :wink:
Yeah, and to be sure, I wasn't getting on Ann's case about that at all (I'm sure her English is orders of magnitude better than my Swedish). And of course, it's common to say it the way she did. But since my work heavily involves orbital dynamics, it's one of those little things that always catches my eye, so it seemed reasonable to point out the more technical usage.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Thu Aug 09, 2012 7:05 pm

ta152h0 wrote:It would be a perfect haperstance if one of your " unsuspecting passerby"s " was a certain Mr Peterson.
I'm sure I would say something stupid, like "elliptical" rather than "eccentric", and need to be corrected. :wink:

Re: APOD: Mars in the Loop (2012 Aug 09)

by waterfeller » Thu Aug 09, 2012 6:19 pm

Chris Peterson wrote:
waterfeller wrote:Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...
Mars stays in the same plane, and Earth stays in the same plane... but they are different planes. So our relative "up and down" positions change with respect to each other.
Of course. With the amazing star background, it is easy to forget that the camera was pointed in a different direction for each picture so we are seeing a different part of the Mars plane, making the "up and down" motion understandable. Out of curiosity, what is the angle between the two planes and when during our year do they intersect?

Re: APOD: Mars in the Loop (2012 Aug 09)

by ta152h0 » Thu Aug 09, 2012 6:16 pm

It would be a perfect haperstance if one of your " unsuspecting passerby"s " was a certain Mr Peterson.

Re: APOD: Mars in the Loop (2012 Aug 09)

by Anthony Barreiro » Thu Aug 09, 2012 5:58 pm

This is an awesome picture. The background stars are so clear and sharp. And you can really see how Mars brightened and grew in apparent diameter as it approached opposition and faded and shrank afterwards. The overlay with the dates and star names is helpful, too.

I've been enjoying pointing out Mars, Saturn, and Spica to unsuspecting passersby and encouraging them to watch Mars move in the sky over the next couple of weeks. You can see Mars moving from one evening to the next. It's a teachable moment, how each star stays in the same place in its constellation, while the planets move through the constellations of the zodiac. And Mars, being closer to the Sun than Saturn, moves through space and through the sky much faster. Next up: Ares and Antares!

Re: APOD: Mars in the Loop (2012 Aug 09)

by StarCuriousAero » Thu Aug 09, 2012 5:46 pm

The two links "retrograde motion" and "can be seen" REALLY helped me visualize what was going on here exactly, I never quite understood when/for how long the retrograde motion actually occurred (one month didn't seem like long enough). Thanks for those!

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Thu Aug 09, 2012 4:49 pm

eturc wrote:I had wondered the same thing and whether it had anything to do with where the photographer was on Earth? Are the different planetary planes in our solar system changing/shifting their angles with respect to one another over time?
The position of the imager on Earth doesn't change the apparent path of Mars.

The planes that planets orbit on change due to precession and perturbations, but these changes have cycles on the order of tens or hundreds of thousands of years, and are thus insignificant in the context of images like today's.

Re: APOD: Mars in the Loop (2012 Aug 09)

by eturc » Thu Aug 09, 2012 4:27 pm

Chris Peterson wrote:
waterfeller wrote:Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...
Mars stays in the same plane, and Earth stays in the same plane... but they are different planes. So our relative "up and down" positions change with respect to each other.
I had wondered the same thing and whether it had anything to do with where the photographer was on Earth? Are the different planetary planes in our solar system changing/shifting their angles with respect to one another over time?

Re: APOD: Mars in the Loop (2012 Aug 09)

by Chris Peterson » Thu Aug 09, 2012 3:24 pm

waterfeller wrote:Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...
Mars stays in the same plane, and Earth stays in the same plane... but they are different planes. So our relative "up and down" positions change with respect to each other.

Re: APOD: Mars in the Loop (2012 Aug 09)

by waterfeller » Thu Aug 09, 2012 3:07 pm

Why is the track of the retrograde motion a loop? Doesn't Mars stay in the same plane? I would think the track would be a straight line with overlap during the retrograde period...

Re: APOD: Mars in the Loop (2012 Aug 09)

by Beyond » Thu Aug 09, 2012 2:31 pm

RJN wrote:
Beyond wrote:Be prepared to wait a while for Curiosity's newest pictures. The picture it took of itself finally came up. The 360' panorama gave a server error, JRun.
Yes. Unexpected. Thanks! I have located alternative links for "360 panorama" and "rover self portrait" which now appear to be quicker to respond. Please try them now. - RJN
Works 'normal' now. Thanks RJN.

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