New Horizons flyby of Pluto [updated for Ultima Thule]

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The New Horizons mission's flyby of Pluto will occur on July 14, 2015, with a significant pause in data transmission until mid-September. During the flyby, New Horizons will prioritize scientific data collection over communication with Earth, resulting in no data being sent back on the flyby day. A recent anomaly caused the spacecraft to switch to a backup computer, leading to an 81-minute communication blackout. The mission's imaging system, LORRI, has a resolution of about 1 arcsecond and will provide critical data on Pluto's surface and atmosphere.

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  • Knowledge of imaging systems, specifically LORRI specifications
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  • #181
OmCheeto said:
Well, I found a gravity bug in my method, yielding somewhat different numbers.

My gravity number is 4 times larger than yours at the Thule end.
Even discounting the gravity from Ultima, my value is still 3 times higher than yours.
g = 1.5e15 kg * 6.674e-11 / (7000 m)^2 = 0.002043 m/s^2

0.002043 / 0.0007 = 2.9


What am I doing wrong?

You are using billiard ball physics but your "centre" of mass seems to be at the point they touch.

If you want to simply to two point masses they are separated by 7+9.5km
If you want the effect of one mass at the outside to the other it's its radius plus the diam of the other.

BTW inverse square law can only be applied "far field" , ie. where the diameters are much smaller than the separation between them.
 
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  • #182
Inverse square law is exact everywhere outside of spherically symmetric objects (within Newtonian mechanics). Didn’t pay much attention to that discussion part so far but if there is still something unclear I can have a look.
 
  • #183
"Inverse square law is exact everywhere outside of spherically symmetric objects"
It is good enough for a first approximation but it is certainly not exact.

Consider a test mass one radius from a spherical body. Work out the contributions form two points diametrically opposed on the surface, once is distant by r , the other by 3r. Compare that to the same masses placed a the centre of mass.

1/r^2+1/(3r)^2 = 2/(2r)^2 ??

A similar inequality and of the same sign will apply for all pairs of points symmetrically placed either side of the plane through the c.o.m. and perpendicular to the line joining the test mass and the centre. Summing all such pairs to represent the whole shows the inequality holds for the whole body.

The inaccuracy reduces as the separation becomes much larger than the diameter of the sphere.
 
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  • #184
It is exact. You can't limit the calculation to two points, you have to integrate over the whole shell. Do it and see what you get.
Alternatively: It is a direct consequence of Gauss' law.

This is a well-known result from classical mechanics and not the topic of this thread. If you have more questions about it please start a separate thread.
 
  • #187
And, we're back in business.

2019.01.08.DSN.NHPC.downloading.png


Not sure how long it will take to download the next image. I guess it depends on how big the file is.
 

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  • #188
Could you post the link to that page, Om?
 
  • #189
Borg said:
Could you post the link to that page, Om?
https://eyes.nasa.gov/dsn/dsn.html

Btw, it's possible they were just checking for a signal when I checked, and got nothing but noise.
Currently, only 3 of the 12 dishes are in use, and New Horizons is not one of them.
 
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  • #190
Canberra (43) is receiving data from New Horizons right now. 2 kb/s downlink at 8.44 GHz, 500 b/s uplink at 7.18 GHz.

Edit: Canberra tweeted it, too
 
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  • #192

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