2019ApJ...877...14Z


Query : 2019ApJ...877...14Z

2019ApJ...877...14Z - Astrophys. J., 877, 14-14 (2019/May-3)

Relativistic astronomy. II. In-flight solution of motion and test of special relativity light aberration.

ZHU J.-P., ZHANG B. and YANG Y.-P.

Abstract (from CDS):

The Breakthrough Starshot project aims to send centimeter-sized, gram-scale "StarChip" probes to Alpha Centauri at a speed of ∼0.2 c. On the other hand, Zhang & Li recently proposed that transrelativistic cameras may be sent to any direction to study astronomical objects and test special relativity. To conduct such "relativistic astronomy," one needs to solve the motion of the probe in flight. We solve the motion of the probe (including the moving direction and the velocity) by comparing the positions of three or more point sources observed in the Earth rest frame and in the probe's comoving frame. When the positions of enough point sources are taken into account, the motion of the probe can be solved with an error that is even smaller than the diffraction limit of the transrelativistic camera. After solving the motion, when the measurement of the position of an additional point source is introduced, one can use the data to test the light aberration effect in special relativity. The upper limit of the photon mass can be placed from the deviation of aberration to slightly lower than the energy of the photon, e.g., ∼1 eV.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): methods: observational

Simbad objects: 33

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Number of rows : 33
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * ups Car * 09 47 06.12170 -65 04 19.2267   3.25 2.99 4.92   A9 77 0
2 * ome Car Be* 10 13 44.2205948661 -70 02 16.463210640 2.92 3.25 3.33 3.29 3.32 B7III 129 0
3 * eps Cru PM* 12 21 21.6081337639 -60 24 04.133270061   4.98 3.57     K3III 97 0
4 * mu.01 Cru Pu* 12 54 35.6242611666 -57 10 40.528916907 3.12 3.87 4.04 4.14 4.38 B2IV-V 159 0
5 * iot Cen PM* 13 20 35.8128156095 -36 42 44.296492410 2.77 2.76 2.73 2.68 2.69 kA1.5hA3mA3Va 218 0
6 HD 121474 PM* 13 57 38.8835769912 -63 41 12.113940624   5.802 4.701     K1.5IIIb: 55 0
7 HD 121901 PM* 14 00 17.3911443816 -61 28 51.698057988   6.793 6.469     F0/2III/IV 36 0
8 HD 125628 * 14 22 37.0730099 -58 27 32.819332   5.79 4.94     G9III 38 0
9 NAME Proxima Centauri PM* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1483 0
10 NAME Proxima Centauri b Pl 14 29 42.9461331854 -62 40 46.164680672           ~ 445 0
11 * rho Lup V* 14 37 53.2261607412 -49 25 32.981831985 3.34 3.90 4.05 4.14 4.25 B3/4V 112 0
12 * alf Cen ** 14 39 36.50 -60 50 02.3   0.4 -0.1     G2V+K1V 1031 0
13 * alf Cir a2* 14 42 30.4206520931 -64 58 30.478845491 3.55 3.43 3.19 2.96 2.86 A7VpSrCrEu 384 0
14 * alf Aps * 14 47 51.7110952914 -79 02 41.112796494   5.247 3.798     K3IIICN0.5 72 0
15 HD 131342 PM* 14 55 34.5596629392 -60 06 50.995267884   6.347 5.180     K2III 35 0
16 * tet Cir Be* 14 56 43.9850523987 -62 46 51.675365388 4.34 5.11 5.11 4.87 4.79 B2III 120 0
17 * kap Lup Be* 15 11 56.0732718648 -48 44 16.169955108 3.55 3.67 3.70 3.75 3.76 B9.5Vne 105 0
18 * phi01 Lup PM* 15 21 48.3695971307 -36 15 40.943845073   5.076 3.546     K4III 103 0
19 * eps Lup bC* 15 22 40.8682566 -44 41 22.614637 2.46 3.191 3.366     B3IV+B3:V 193 0
20 * eps Oph PM* 16 18 19.2902245358 -04 41 33.047349888 4.95 4.21 3.23 2.54 2.05 G9.5IIIbFe-0.5 246 0
21 * gam02 Nor PM* 16 19 50.4223079953 -50 09 19.821590813 6.27 5.10 4.02 3.24 2.66 K0III 78 0
22 * eta Ara * 16 49 47.1562913570 -59 02 28.965649640   5.306 3.744     K5III 74 0
23 * 36 Oph ** 17 15 20.9839376 -26 36 10.157115           K2V+K1V 145 0
24 * bet Ara s*r 17 25 17.9878053183 -55 31 47.574076000 5.87 4.31 2.85     K0/1Ib 139 0
25 * bet Oph PM* 17 43 28.3519097803 +04 34 02.293206489 5.150 3.930 2.750 1.96 1.38 K2IIICN0.5 490 0
26 * eta Pav PM* 17 45 43.9875971845 -64 43 25.937272871   4.769 3.581     K2II 54 0
27 * bet Sct SB* 18 47 10.4742156840 -04 44 52.342960488 6.15 5.31 4.22 3.43 2.86 G4IIa 194 0
28 * ksi02 Sgr * 18 57 43.8001892867 -21 06 23.967339435 5.82 4.69 3.51 2.71 2.12 G8/K0II/III 123 0
29 * chi01 Sgr ** 19 25 16.4906536621 -24 30 30.841584088   5.238 5.009 6.67   A3/5IV/V 79 0
30 * mu. Aql PM* 19 34 05.3529921054 +07 22 44.184329526 6.87 5.63 4.45 3.55 2.94 K3-IIIbFe0.5 272 1
31 * bet01 Cap SB* 20 21 00.6665981712 -14 46 53.067367488 4.14 3.87 3.08 2.53 2.03 G9II:+B8p:Si: 192 0
32 * eps Cyg ** 20 46 12.6722768426 +33 58 13.182037125 4.370 3.520 2.480 1.73 1.19 K0III 519 0
33 * eps Peg LP* 21 44 11.1561394 +09 52 30.031152 5.61 3.91 2.39 1.34 0.58 K2Ib-II 464 1

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