viernes, 30 de enero de 2015

Talking to Pluto is hard! Why it takes so long to get data back from New Horizons

Talking to Pluto is hard! Why it takes so long to get data back from New Horizons

Posted by Emily Lakdawalla

2015/01/30 15:53 UTC

Topics: New Horizons, mission status, explaining technology

As I write this post, New Horizons is nearing the end of a weeklong optical navigation campaign. By taking photos of the Pluto system at regular intervals, New Horizons' navigators can precisely measure the observed positions of Pluto and its moons with respect to background stars, and determine the spacecraft's position. The last optical navigation images in the weeklong series will be taken tomorrow, but it will likely take two weeks or more for all the data to get to Earth. Two weeks! Why does it take so long? It's not like it's all that much data: 10 full-resolution LORRI images per day.

The short answer to that question is: Pluto is far away -- very far away, more than 30 times Earth's distance from the Sun -- so New Horizons' radio signal is weak. Weak signal means low data rates: at the moment, New Horizons can transmit at most 1 kilobit per second. (Note that spacecraft communications are typically measured in bits, not bytes; 1 kilobit is only 125 bytes.) Even at these low data rates, only the Deep Space Network's very largest, 70-meter dishes can detect New Horizons' faint signal.

DSS-43, the 70-meter dish at Canberra, Australia

Glen Nagle

DSS-43, the 70-meter dish at Canberra, Australia
Taken on November 10, 2011 while the Sun was surrounded by a "sunbow."

How much data is in a single LORRI image? (LORRI, which stands for Long Range Reconnaissance Imager, is New Horizons' highest-resolution camera.) LORRI's detector is 1024 pixels square. Like many modern space cameras, when the camera reads out its detector, it digitizes each pixel as a 12-bit number. Twelve million is an awful lot of bits, but fortunately LORRI's images are amenable to lossless compression, especially now when they contain mostly black space; they can be zipped up to about 2.5 Megabits without any loss of detail. They can be made even smaller with lossy JPEG compression, but for optical navigation, precision counts; the pictures have to be returned losslessly.

So, do the math. 2.5 Megabits, at 1 kilobit per second: it takes 42 minutes to return one LORRI photo to Earth. Most communications sessions last about eight hours. That's eleven images per communications session. And that assumes that New Horizons is transmitting only LORRI data, which it's not; there are other science instruments and spacecraft housekeeping data, too. The Deep Space Network has only three 70-meter dishes, and there is a lot of competition for time on them; New Horizons is lucky to get one communications session per day. And while New Horizons is pointing its dish at Earth, it can't point at anything else, including Pluto. It has to choose between communicating and taking data.

What all of this means is that whenever New Horizons is actively taking science data, it's building up a data backlog, which it fails to transmit completely in its next communications session. The New Horizons team wants to go into the close encounter phase with data recorders as empty as possible, clearing the decks for all that juicy data from the flyby. What to do?

They have a neat trick that can nearly double New Horizons' data transmission rate, but it comes at a cost of doing simultaneous science. New Horizons' radio system includes two Traveling Wave Tube Amplifiers or TWTAs (pronounced "twittas," like a Bostonian would say "twitters"). The TWTAs amplify the radio signals before they get broadcast from New Horizons' 2.1-meter dish. There are two TWTAs for redundancy: if one fails, the mission will still be able to return data to Earth. But the two TWTAs are not quite identical. One of them transmits radio signals with left-hand circular polarization, and one of them transmits with right-hand circular polarization.

Because they transmit with different polarization, both TWTAs can simultaneously transmit the same data through the dish antenna. On Earth, special hardware at the Deep Space Network can separately receive the two differently-polarized signals, and then combine them to make the signal stronger. Stronger signal means New Horizons can transmit at a higher data rate, about 1.9 times the rate with a single TWTA.

This two-TWTA mode wasn't developed until after launch; they deployed it early in the mission, and it worked well. But radio transmitters are power-hungry. New Horizons' nuclear power source has decayed since it launched nearly a decade ago, and there is no longer enough power to run both TWTAs at the same time as all the other spacecraft subsystems. If they want to nearly double their data rate and reduce their backlog, they need to shut something else down.

Amazingly, they can shut down their guidance and control system and use the saved power to run the second transmitter. But how can you point stably at Earth with your guidance system shut down? The answer is to turn New Horizons from a spacecraft whose orientation stays fixed in space to one that spins. Spinning spacecraft have incredibly stable pointing. It's costly in terms of precious hydrazine fuel to spin up and spin down the spacecraft, so they don't want to make the transition from three-axis to spin-stabilized very often. And you can't take photos from a spinning spacecraft (not with the cameras New Horizons has, anyway). But it's worth it to spend a little hydrazine and quit taking pictures a couple of times in order to get all the approach data down to Earth before the near-encounter phase starts.

So that's why New Horizons is going to spend two long periods of its Pluto approach taking no image data, with the spacecraft spinning and its high-gain antenna pointed at Earth. The two spin periods are scheduled right after trajectory correction maneuvers, rocket-firings that will fine-tune New Horizons' path past Pluto. The first spin period will last from March 10 to April 4; the second lasts from May 15 to May 27. For image fans like me, it'll be a little frustrating to know that Pluto will be getting bigger and bigger, yet New Horizons is not looking. But the consolation is that New Horizons will completely empty its memory on both occasions, sending everything it's got back to Earth, and making room for more and better data. And while the spacecraft is spinning, its particles instruments SWAP, PEPSSI, and SDC can all still take data.

 

New Horizons should be able to use this two-TWTA communication mode until well after the flyby, assuming, of course, that both transmitters remain healthy. It'll still take more than a year to get all the science data from the encounter back to Earth; it's a lot of data, and a skinny pipe. And it won't be able to use the two-TWTA communication mode forever. Eventually, the output of the nuclear power supply will decay to the point that even while spinning, New Horizons won't have enough power to run both transmitters simultaneously, and we'll be back to using just one at a time. The Kuiper belt object flyby will almost certainly require data return through only one transmitter. New Horizons is a lesson in patience!

 

domingo, 18 de enero de 2015

Objetos transneptunianos sugieren que hay más planetas en el Sistema Solar

Objetos transneptunianos sugieren que hay más planetas en el Sistema Solar

 

 

Makemake

Ilustración artística del planeta enano Makemake, un objeto transneptuniano. Crédito: IAU, M. Kornmesser (ESA/Hubble).

Los astrónomos llevan décadas debatiendo si queda algún oscuro planeta que descubrir dentro del Sistema Solar más allá de Plutón. Según los cálculos de científicos de la Universidad Complutense de Madrid (UCM) y la Universidad de Cambridge (Reino Unido), al menos dos planetas deben existir para explicar el comportamiento de los objetos transneptunianos extremos (ETNO).

La teoría establece que estos objetos que se mueven mucho más allá de Neptuno deberían distribuirse de forma aleatoria, y por un sesgo observacional, su órbita debe cumplir una serie de características: tener un semieje mayor con un valor de unas 150 UA (unidades astronómicas, o la distancia entre la Tierra y el Sol), una inclinación casi de 0° y un argumento o ángulo del perihelio (punto de la órbita más próximo a nuestra estrella) también cercano a 0° o a 180°.

Pero lo que se observa en una docena de estos cuerpos es bastante diferente: los valores del semieje mayor son muy dispersos (entre 150 UA y 525 UA), la inclinación media de la órbita ronda los 20° y su argumento del perihelio es de unos -31°, sin aparecer ni un solo caso cercano a 180°.

“Este exceso de objetos con parámetros orbitales distintos a los esperados nos hace pensar que algunas fuerzas invisibles están alterando la distribución de los elementos orbitales de los ETNO, y consideramos que la explicación más probable es que existen planetas desconocidos más allá de Neptuno y Plutón”, explica Carlos de la Fuente Marcos, científico de la UCM y coautor del trabajo.

“El número exacto es incierto, dado que los datos que tenemos son limitados, pero nuestros cálculos sugieren que por lo menos hay dos planetas, y probablemente más, en los confines de nuestro sistema solar”, añade el astrofísico.

Para realizar su estudio, los investigadores han analizado los efectos del denominado mecanismo Kozai, relacionado con la perturbación gravitacional que ejerce un cuerpo grande sobre la órbita de otro mucho más pequeño y lejano. Como referencia han considerado como funciona este mecanismo en el caso del cometa 96P/Machholz 1 por la influencia de Júpiter.

Dos problemas que resolver

A pesar de sus sorprendentes resultados, los autores reconocen que sus datos se enfrentan a dos problemas. Por un lado, su planteamiento está en contra de lo que predicen los modelos actuales de formación del Sistema Solar, que aseguran que no pueden existir planetas moviéndose en órbitas circulares más allá de Neptuno.

Sin embargo, el reciente descubrimiento del radiotelescopio ALMA de un disco de formación de planetas a más de 100 unidades astronómicas de la estrella HL Tauri, más joven y de menor masa que el Sol, sugiere que sí se pueden formar planetas a varios centenares de unidades astronómicas del centro del sistema.

Por otra parte, el equipo reconoce que su análisis está basado en una muestra con pocos objetos (13, concretamente), pero adelantan que en los próximos meses se van a hacer públicos más resultados con una muestra mayor. “Si se confirma, nuestro resultado puede ser realmente revolucionario en astronomía”, apunta De la Fuente Marcos.

El año pasado dos investigadores estadounidenses también descubrieron un planeta enano llamado 2012 VP113 en la nube de Oort, justo más allá de nuestro sistema solar. Los descubridores consideran que su órbita se ve influenciada por la posible presencia de una súper-Tierra oscura y gélida, de un tamaño hasta diez veces el de nuestro planeta.

El estudio “Flipping minor bodies: what comet 96P/Machholz 1 can tell us about the orbital evolution of extreme trans-Neptunian objects and the production of near-Earth objects on retrograde orbits” fue publicado en la edición del 11 de enero de 2015 deMonthly Notices of the Royal Astronomical Society.

El artículo “Extreme trans-Neptunian objects and the Kozai mechanism: signalling the presence of trans-Plutonian planets” fue publicado en la edición del 1 de septiembre de 2014 de Monthly Notices of the Royal Astronomical Society Letters.

Fuente: SINC

viernes, 9 de enero de 2015

Will the Real Monster Black Hole Please Stand Up?

Will the Real Monster Black Hole Please Stand Up?
 
January 8, 2015
 

 

Colliding galaxies Arp 299
The real monster black hole is revealed in this new image from NASA's Nuclear Spectroscopic Telescope Array of colliding galaxies Arp 299. In the center panel, the NuSTAR high-energy X-ray data appear in various colors overlaid on a visible-light image from NASA's Hubble Space Telescope.
Image Credit: 
NASA/JPL-Caltech/GSFC
 

 

A new high-energy X-ray image from NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, has pinpointed the true monster of a galactic mashup. The image shows two colliding galaxies, collectively called Arp 299, located 134 million light-years away. Each of the galaxies has a supermassive black hole at its heart.

 

NuSTAR has revealed that the black hole located at the right of the pair is actively gorging on gas, while its partner is either dormant or hidden under gas and dust.

 

The findings are helping researchers understand how the merging of galaxies can trigger black holes to start feeding, an important step in the evolution of galaxies.

 

"When galaxies collide, gas is sloshed around and driven into their respective nuclei, fueling the growth of black holes and the formation of stars," said Andrew Ptak of NASA's Goddard Space Flight Center in Greenbelt, Maryland, lead author of a new study accepted for publication in the Astrophysical Journal. "We want to understand the mechanisms that trigger the black holes to turn on and start consuming the gas."

 

NuSTAR is the first telescope capable of pinpointing where high-energy X-rays are coming from in the tangled galaxies of Arp 299. Previous observations from other telescopes, including NASA's Chandra X-ray Observatory and the European Space Agency's XMM-Newton, which detect lower-energy X-rays, had indicated the presence of active supermassive black holes in Arp 299. However, it was not clear from those data alone if one or both of the black holes was feeding, or "accreting," a process in which a black hole bulks up in mass as its gravity drags gas onto it.

 

The new X-ray data from NuSTAR -- overlaid on a visible-light image from NASA's Hubble Space Telescope -- show that the black hole on the right is, in fact, the hungry one. As it feeds on gas, energetic processes close to the black hole heat electrons and protons to about hundreds of millions of degrees, creating a superhot plasma, or corona, that boosts the visible light up to high-energy X-rays. Meanwhile, the black hole on the left either is "snoozing away," in what is referred to as a quiescent, or dormant state, or is buried in so much gas and dust that the high-energy X-rays can't escape.

 

"Odds are low that both black holes are on at the same time in a merging pair of galaxies," said Ann Hornschemeier, a co-author of the study who presented the results Thursday at the annual American Astronomical Society meeting in Seattle. "When the cores of the galaxies get closer, however, tidal forces slosh the gas and stars around vigorously, and, at that point, both black holes may turn on."

 

NuSTAR is ideally suited to study heavily obscured black holes such as those in Arp 299. High-energy X-rays can penetrate the thick gas, whereas lower-energy X-rays and light get blocked.

 

Ptak said, "Before now, we couldn't pinpoint the real monster in the merger."

 

NuSTAR is a Small Explorer mission led by the California Institute of Technology in Pasadena and managed by NASA's Jet Propulsion Laboratory, also in Pasadena, for NASA's Science Mission Directorate in Washington. The spacecraft was built by Orbital Sciences Corporation, Dulles, Virginia. Its instrument was built by a consortium including Caltech; JPL; the University of California, Berkeley; Columbia University, New York; NASA's Goddard Space Flight Center, Greenbelt, Maryland; the Danish Technical University in Denmark; Lawrence Livermore National Laboratory, Livermore, California; ATK Aerospace Systems, Goleta, California, and with support from the Italian Space Agency (ASI) Science Data Center.

 

NuSTAR's mission operations center is at UC Berkeley, with the ASI providing its equatorial ground station located at Malindi, Kenya. The mission's outreach program is based at Sonoma State University, Rohnert Park, California. NASA's Explorer Program is managed by Goddard. JPL is managed by Caltech for NASA.

 

NASA is exploring our solar system and beyond to understand the universe and our place in it. The agency seeks to unravel the secrets of our universe, its origins and evolution, and search for life among the stars.

 

For more information, visit http://www.nasa.gov/nustar and http://www.nustar.caltech.edu/ .

 

Whitney Clavin
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-4673
whitney.clavin@jpl.nasa.gov

2015-007