Invite Ross 128 Over This Thanksgiving

Total Page:16

File Type:pdf, Size:1020Kb

Load more

Invite Ross 128 Over This Thanksgiving By: Bob King | November 22, 2017 With exoplanet Ross 128b in the news, we pay a visit to the star that sustains this potentially habitable exoplanet. The red dwarf, Ross 128, hosts the temperate, Earth-sized planet Ross 128 b. The star is about 20% of the Sun's diameter and 17% as massive. Sloan Digital Sky Survey No matter where you look the fecundity of the universe is manifest. Consider exoplanets. Since the first was discovered in 1992, astronomers have been piling them on like mashed potatoes at Thanksgiving. Today we know of more than 3,700. Of those, 53 may be potentially habitable. The most recently discovered potentially life-friendly planet — and in some ways the most exciting — is Ross 128b, which circles the red dwarf star Ross 128 in the constellation Virgo. Located just 11 light-years away, it's the second closest Earth-sized planet within the habitable zone of its star. Astronomers estimate that temperatures on Ross 128b range from –76° to 68° F (–60° to 20° C). You could argue that's even more temperate than than that of Earth and likely warm enough for liquid water to pool on its surface. What's more, its star experiences far fewer massive flares compared to other red dwarfs, making conditions more hospitable to potential life. If you have a 4.5-inch or larger telescope, you can track down Ross 128 in Virgo in the morning sky. Place Beta (β) Virginis in the field of a low-power eyepiece and you're halfway there! Mars's location is shown for November 21st. Stellarium While you and I aren't going to see Ross 128b anytime soon, we can have the pleasure of seeing its host sun, Ross 128. Currently visible in a dark sky before the start of dawn, this newsy red dwarf is just 1.1° southwest of 3rd-magnitude Beta (β) Virginis. To find the dwarf and its mind's-eye planet, center Beta in the field of view and use the AAVSO map to star-hop right to it. Once Beta (β) Vir is in the field of view, use this chart from the American Association. of Variable Star Observers to star-hop to Ross 128, also known as the variable star FI Virginis. Numbers are stellar magnitudes with the decimals omitted, so 107 = 10.7. North is up. AAVSO with annotations by the author Eager to see it for myself, I got up the first clear morning after the news of the discovery broke last week. Oh gosh, how easy could it be. Pale red and magnitude 11.2, Ross 128 is bright enough to spot in telescopes as small as 4 inches (10 cm). Mingled in the star's light were photons from its closely orbiting and perhaps habitable planet, a satisfying thought. Some 80% of the Milky Way's stars are red dwarfs, yet not a single one is visible to the naked eye. Being something of an introvert, I cotton to these shy suns. The brightest, Lacaille 8760 in Microscopium, shines at magnitude 6.7. Despite their retiring nature, they make for fertile exoplanet hunting grounds. A tiny dwarf feels a much stronger — and more easily measurable — tug by an orbiting planet compared to a bigger star like our Sun. This graph shows how the distances of several nearby stars change over a period from 20,000 years in the past to 80,000 years in the future. “0” is the current time; distances are given in light years. Ross 128 is closing in, as is Alpha Centauri. Around the year 25,000 AD, the Alpha Centauri system will be just 3 light-years from Earth. FrancescoA / CC SA-3.0 If we're patient and smart enough not to destroy ourselves, we'll have an even better view of Ross 128 in due time. The star is moving towards us at 31 km/sec and will become our nearest stellar neighbor around 81,000 AD, when only 6.2 light-years will separate the two Earths. We celebrate Thanksgiving this week, a time to be grateful for all we have. As we reflect on the ups and downs that sustain our lives, feel free to take another helping at the table, including this stellar cranberry. CATEGORIES Explore the Night with Bob King, Observing, Observing News & Current Celestial Events, Variable Stars TAGS Exoplanets RELATED POSTS Puffed-Up Hot Jupiter Is Surprisingly Dark New Star and Exoplanet Names OK’d by IAU Exoplanet Portraits: A Tale of New Instruments Three Exoplanet Molds: Metals Matter Exoplanet Out for a Quick Spin About Bob King Amateur astronomer since childhood and long-time member of the American Association of Variable Star Observers (AAVSO), Bob King also teaches community education astronomy and writes the blog Astro Bob. The universe invites us on an adventure every single night. All we need do is look up. My book "Night Sky with the Naked Eye" was just published and is now available on Amazon and BN. It covers all the great things you can see at night with just your eyeballs. No equipment needed! .
Recommended publications
  • Temperature-Spectral Class-Color Index Relationships for Main

    Temperature-Spectral Class-Color Index Relationships for Main

    ASTRONOMY SURVIVAL NOTEBOOK Stellar Evolution SESSION FOURTEEN: THE EVOLUTION OF STARS Approximate Characteristics of Several Types of MAIN SEQUENCE STARS Mass in Contraction Surface Luminosity M Years on Radius Class Comparison to Zero Age Temp. compared Absolute Main in to Sun Main Sequence (K) to sun Magnitude Sequence suns Not well known O6 29.5 10 Th 45,000 140,000 -4.0 2 M 6.2 mid blue super g O9 22.6 100 Th 37,800 55,000 -3.6 4 M 4.7 late blue super g B2 10.0 400 Th 21,000 3,190 -1.9 30 M 4.3 early B5 5.46 1 M 15,200 380 -0.4 140 M 2.8 mid A0 2.48 4 M 9,600 24 +1.5 1B 1.8 early A7 1.86 10 M 7,920 8.8 +2.4 2 B 1.6 late F2 1.46 15 M 7,050 3.8 +3.8 4 B 1.3 early G2 1.00 20 M 5,800 1.0 +4.83 10 B 1.0 early sun K7 0.53 40 M 4,000 0.11 +8.1 50 B 0.7 late M8 0.17 100 M 2,700 0.0020 +14.4 840B 0.2 late minimum 2 Jupiters Temperature-Spectral Class-Color Index Relationships for Main-Sequence Stars Temp 54,000 K 29,200 K 9,600 K 7,350 K 6,050 K 5,240 K 3,750 K | | | | | | | Sp Class O5 B0 A0 F0 G0 K0 M0 Co Index (UBV) -0.33 -0.30 -0.02 +0.30 +0.58 +0.81 +1.40 1.
  • The Constellation Microscopium, the Microscope Microscopium Is A

    The Constellation Microscopium, the Microscope Microscopium Is A

    The Constellation Microscopium, the Microscope Microscopium is a small constellation in the southern sky, defined in the 18th century by Nicolas Louis de Lacaille in 1751–52 . Its name is Latin for microscope; it was invented by Lacaille to commemorate the compound microscope, i.e. one that uses more than one lens. The first microscope was invented by the two brothers, Hans and Zacharius Jensen, Dutch spectacle makers of Holland in 1590, who were also involved in the invention of the telescope (see below). Lacaille first showed it on his map of 1756 under the name le Microscope but Latinized this to Microscopium on the second edition published in 1763. He described it as consisting of "a tube above a square box". It contains sixty-nine stars, varying in magnitude from 4.8 to 7, the lucida being Gamma Microscopii of apparent magnitude 4.68. Two star systems have been found to have planets, while another has a debris disk. The stars that now comprise Microscopium may formerly have belonged to the hind feet of Sagittarius. However, this is uncertain as, while its stars seem to be referred to by Al-Sufi as having been seen by Ptolemy, Al-Sufi does not specify their exact positions. Microscopium is bordered Capricornus to the north, Piscis Austrinus and Grus to the west, Sagittarius to the east, Indus to the south, and touching on Telescopium to the southeast. The recommended three-letter abbreviation for the constellation, as adopted Seen in the 1824 star chart set Urania's Mirror (lower left) by the International Astronomical Union in 1922, is 'Mic'.
  • The Hertzsprung - Russell Diagram Today You Will Be Making the Hertzsprung - Russell Diagram

    The Hertzsprung - Russell Diagram Today You Will Be Making the Hertzsprung - Russell Diagram

    Name: ___________________________________ The Hertzsprung - Russell diagram Today you will be making the Hertzsprung - Russell diagram. The H-R diagram allows astronomers to classify stars into groups. The two axes for this graph will be temperature and magnitude. When we refer to temperature, we are talking about the surface of the star. The surface temperature is much cooler. For example, our sun’s surface temperature is ~5,500K to 6,000 K. Kelvin is a temperature scale very similar to Celsius. Absolute magnitude is a measurement of how bright a star really is. This is determined by its size and by its temperature. Even though it might look bright in our sky, we try to compare all stars as if we were standing the exact same distance away from each one. This magnitude value is stated by calculating how bright the object would shine at a fixed distance away in space, ~32.6 light years (10 parsecs for those wanting another measurement to think about). Main sequence stars Temperature Magnitude Red Giant stars Temperature Magnitude Bellatrix 18000 -2.0 Capella 5000 -0.6 Regulus 12000 -0.6 Pollux 4650 0.8 Spica 19500 -2.0 Arcturus 4500 -0.3 Beta Centauri 21000 -3.0 Aldebaran 3900 -0.2 Achernar 16500 -3.0 Beta Tauri 12000.0 -2 Beta Crucis 21000.0 -3.9 Red Super Giant Alpha Crucis 19500.0 -4 Rigel 11000 -6.8 Vega 9750 0.5 Deneb 8500 -6.9 Castor 9250 0.9 Canopus 7400 -3.1 Beta Carinae 9750.0 -0.4 Antares 3500 -4.5 Sirius A 9250.0 1.5 Betelgeuse 3200 -5.5 Formalhaut 8500 2.0 Altair 7750 2.2 White Dwarfs Procyon A 6500 2.6 Sirius B 8100 11.4 Alpha Centauri A 5750 4.4 Procyon B 6500 13.1 Sun 5750 4.9 Tau Ceti 5344 5.7 Epsilon Eridani 4500 6.1 Epsilon Indi 4250 7 Cygni A 3800 7.5 Cygni B 3700 8 Alpha Centauri B 3900 5.8 Kapteyn's Star 3400 11.2 Lacaille 8760 3200 8.8 Lacaille 21185 3000 10.5 Bernard's Star 2600 13.2 Ross 614A 2500 13.3 Kruger 60B 2500 13.4 Ross 248 2800 14.7 Use the data on the previous page to plot an H-R diagram.
  • Faint Objects in Motion: the New Frontier of High Precision Astrometry

    Faint Objects in Motion: the New Frontier of High Precision Astrometry

    White paper for the Voyage 2050 long-term plan in the ESA Science Programme Faint objects in motion: the new frontier of high precision astrometry Contact Scientist: Fabien Malbet Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) Université Grenoble Alpes, CS 40700, F-38058 Grenoble cedex 9, France Email: [email protected], Phone: +33 476 63 58 33 version 20190805 Faint objects in motion : the new frontier of high precision astrometry Faint objects in motion: the new on the most critical questions of cosmology, astron- frontier of high precision astrometry omy and particle physics. Sky survey telescopes and powerful targeted telesco- 1.1 Dark matter pes play complementary roles in astronomy. In order to The current hypothesis of cold dark matter (CDM) ur- investigate the nature and characteristics of the mo- gently needs verification. Dark matter (DM) is essential tions of very faint objects, a flexibly-pointed instrument to the L + CDM cosmological model (LCDM), which suc- capable of high astrometric accuracy is an ideal comple- cessfully describes the large-scale distribution of galax- ment to current astrometric surveys and a unique tool for ies and the angular fluctuations of the Cosmic Microwave precision astrophysics. Such a space-based mission Background, as confirmed by the ESA / Planck mission. will push the frontier of precision astrometry from ev- Dark matter is the dominant form of matter (∼ 85%) in idence of earth-massed habitable worlds around the the Universe, and ensures the formation and stability of nearest starts, and also into distant Milky way objects enmeshed galaxies and clusters of galaxies.
  • The Detectability of Nightside City Lights on Exoplanets

    The Detectability of Nightside City Lights on Exoplanets

    Draft version September 6, 2021 Typeset using LATEX twocolumn style in AASTeX63 The Detectability of Nightside City Lights on Exoplanets Thomas G. Beatty1 1Department of Astronomy and Steward Observatory, University of Arizona, Tucson, AZ 85721; [email protected] ABSTRACT Next-generation missions designed to detect biosignatures on exoplanets will also be capable of plac- ing constraints on the presence of technosignatures (evidence for technological life) on these same worlds. Here, I estimate the detectability of nightside city lights on habitable, Earth-like, exoplan- ets around nearby stars using direct-imaging observations from the proposed LUVOIR and HabEx observatories. I use data from the Soumi National Polar-orbiting Partnership satellite to determine the surface flux from city lights at the top of Earth's atmosphere, and the spectra of commercially available high-power lamps to model the spectral energy distribution of the city lights. I consider how the detectability scales with urbanization fraction: from Earth's value of 0.05%, up to the limiting case of an ecumenopolis { or planet-wide city. I then calculate the minimum detectable urbanization fraction using 300 hours of observing time for generic Earth-analogs around stars within 8 pc of the Sun, and for nearby known potentially habitable planets. Though Earth itself would not be detectable by LUVOIR or HabEx, planets around M-dwarfs close to the Sun would show detectable signals from city lights for urbanization levels of 0.4% to 3%, while city lights on planets around nearby Sun-like stars would be detectable at urbanization levels of & 10%. The known planet Proxima b is a particu- larly compelling target for LUVOIR A observations, which would be able to detect city lights twelve times that of Earth in 300 hours, an urbanization level that is expected to occur on Earth around the mid-22nd-century.
  • Basics of Astrophysics Revisited. I. Mass- Luminosity Relation for K, M and G Class Stars

    Basics of Astrophysics Revisited. I. Mass- Luminosity Relation for K, M and G Class Stars

    Basics of astrophysics revisited. I. Mass- luminosity relation for K, M and G class stars Edgars Alksnis [email protected] Small volume statistics show, that luminosity of slow rotating stars is proportional to their angular momentums of rotation. Cause should be outside of standard solar model. Slow rotating giants and dim dwarfs are not out of „main sequence” in this concept. Predictive power of stellar mass-radius- equatorial rotation speed-luminosity relation has been offered to test in numerous examples. Keywords: mass-luminosity relation, stellar rotation, stellar mass prediction, stellar rotation prediction ...Such vibrations would proceed from deep inside the sun. They are a fast way of transporting large amounts of energy from the interior to the surface that is not envisioned in present theory.... They could stir up the material inside the sun, which current theory tends to see as well layered, and that could affect the fusion dynamics. If they come to be generally accepted, they will require a reworking of solar theory, and that carries in its train a reworking of stellar theory generally. These vibrations could reverberate throughout astronomy. (Science News, Vol. 115, April 21, 1979, p. 270). Actual expression for stellar mass-luminosity relation (fig.1) Fig.1 Stellar mass- luminosity relation. Credit: Ay20. L- luminosity, relative to the Sun, M- mass, relative to the Sun. remain empiric and in fact contain unresolvable contradiction: stellar luminosity basically is connected with their surface area (radius squared) but mass (radius in cube) appears as a factor which generate luminosity. That purely geometric difference had pressed astrophysicists to place several classes of stars outside of „main sequence” in the frame of their strange theoretic constructions.
  • Effects of Rotation Arund the Axis on the Stars, Galaxy and Rotation of Universe* Weitter Duckss1

    Effects of Rotation Arund the Axis on the Stars, Galaxy and Rotation of Universe* Weitter Duckss1

    Effects of Rotation Arund the Axis on the Stars, Galaxy and Rotation of Universe* Weitter Duckss1 1Independent Researcher, Zadar, Croatia *Project: https://www.svemir-ipaksevrti.com/Universe-and-rotation.html; (https://www.svemir-ipaksevrti.com/) Abstract: The article analyzes the blueshift of the objects, through realized measurements of galaxies, mergers and collisions of galaxies and clusters of galaxies and measurements of different galactic speeds, where the closer galaxies move faster than the significantly more distant ones. The clusters of galaxies are analyzed through their non-zero value rotations and gravitational connection of objects inside a cluster, supercluster or a group of galaxies. The constant growth of objects and systems is visible through the constant influx of space material to Earth and other objects inside our system, through percussive craters, scattered around the system, collisions and mergers of objects, galaxies and clusters of galaxies. Atom and its formation, joining into pairs, growth and disintegration are analyzed through atoms of the same values of structure, different aggregate states and contiguous atoms of different aggregate states. The disintegration of complex atoms is followed with the temperature increase above the boiling point of atoms and compounds. The effects of rotation around an axis are analyzed from the small objects through stars, galaxies, superclusters and to the rotation of Universe. The objects' speeds of rotation and their effects are analyzed through the formation and appearance of a system (the formation of orbits, the asteroid belt, gas disk, the appearance of galaxies), its influence on temperature, surface gravity, the force of a magnetic field, the size of a radius.
  • 44 Closest Stars and How They Compare to Our Sun

    44 CLOSEST STARS AND HOW THEY COMPARE TO OUR SUN R = Solar radius (a unit of distance to express the size of stars relative to the sun) L = Solar luminosity (a unit of radiant flux used SUN System/constellation to compare the luminosity of stars, galaxies, Solar System Potential planets and other celestial objects in terms of the sunʼs output) 8 Distance From Earth 8.317 light-minutes EARTH 1R (432,288 miles) s) -year (light Proxima Centauri TH EAR Alpha Centauri OM E FR 1 ANC DIST 4.244 light-years 0.001 0.01 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10 25 0.1542R 0.00005L L <=0.0001 α Centauri A (Rigil Kentaurus) 1 Alpha Centauri L 4.365 light-years 1.223R 1.519 L α Centauri B (Toliman) 5 Alpha Centauri light-years 4.37 light-years 0.863R 0.5002L Bernard’s Star Ophiuchus 1 5.957 light-years 0.196R 0.0035L Wolf 359 (CN Leonis) Leo 2 7.856 light-years 0.16R 0.0014L Lalande 21185 Ursa Major 1 8.307 light-years 0.393R 0.026L Sirius A Canis Major Luyten 726-8A 8.659 light-years Cetus 1.711 R 25.4L 8.791 light-years 0.14R 0.00004L Sirius B Canis Major 8.659 light-years Luyten 726-8B 0.0084R 0.056L Cetus 8.791 light-years 0.14R 0.00004L Ross 154 Sagittarius 9.7035 light-years 0.24R 0.0038L 10 light-years Epsilon Eridani Eridanus Ross 248 2 Andromeda 10.446 light-years 10.2903 light-years 0.735R 0.34L 0.16R 0.0018L Lacaille 9352 Piscis Austrinus 3 10.7211 light-years Ross 128 0.47R 0.0367L Virgo 1 EZ Aquarii A 11 light-years Aquarius 61 Cygni A 0.1967R 0.00362L 11.1 light-years Cygnus 0.175R 0.000087L 3 (part of triple star system) 11.4 light-years
  • Wyatt, Stanley P., Jr. TITLE the Life Story of a Star, Book 5. Guidebook

    Wyatt, Stanley P., Jr. TITLE the Life Story of a Star, Book 5. Guidebook

    DOCUHEET RESUME ED 196 671 SE 033 213 AUTHOR Atkin, J. Myron; Wyatt, Stanley P., Jr. TITLE The Life Story of a Star, Book 5. Guidebook. The University of Illinois Astronomy Project. INSTITUTION Illinois Univ., Urbana. SPONS AGENCY National Science Foundation, Washington, D.C. PUB DATE 69 NOTE 65p.: For related documents,see SE 033 210-212. EDFS PRICE MF01/PC03 Plus Postage. DESCRIPTORS *Astronomy; Elementary Education; Elementary School Science; Junior High Schools; *Physical Sciences; Science Activities; *Science Curriculum; Science Education; Science History: *Science Programs IDENTIFIERS *Stars: *University of Illinois Astronomy Program ABSTRACT Presented is book five in a series of six books in the University of Illinois Astronomy Program whichintroduces astronomy to upper elementary and junior high schoolstudents. This guidebcok discusses the interior of stars, theirsource of energy, and their evolution. Topics presented include: the physical properties of the sun: model of the solar interior;using known physical laws as guides; the source of solarenergy; properties of stars - their luminosities: temperatures;masses; stellar models; the evolution of stars: mid birth and death of stars.(Author/DS) *********************************************************************** Reproductions supplied by EDRS are the best thatcan be made from the original document. *********************************************************************** THE UNIVERSITY OF ILLINOIS ASTRONOMYPROGRAM THE LIFE STORY OFA STAR CODIRECTORS: J. MYRON ATKIN STANLEYP. WYATT,
  • The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide

    The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide

    The COLOUR of CREATION observing and astrophotography targets “at a glance” guide. (Naked eye, binoculars, small and “monster” scopes) Dear fellow amateur astronomer. Please note - this is a work in progress – compiled from several sources - and undoubtedly WILL contain inaccuracies. It would therefor be HIGHLY appreciated if readers would be so kind as to forward ANY corrections and/ or additions (as the document is still obviously incomplete) to: [email protected]. The document will be updated/ revised/ expanded* on a regular basis, replacing the existing document on the ASSA Pretoria website, as well as on the website: coloursofcreation.co.za . This is by no means intended to be a complete nor an exhaustive listing, but rather an “at a glance guide” (2nd column), that will hopefully assist in choosing or eliminating certain objects in a specific constellation for further research, to determine suitability for observation or astrophotography. There is NO copy right - download at will. Warm regards. JohanM. *Edition 1: June 2016 (“Pre-Karoo Star Party version”). “To me, one of the wonders and lures of astronomy is observing a galaxy… realizing you are detecting ancient photons, emitted by billions of stars, reduced to a magnitude below naked eye detection…lying at a distance beyond comprehension...” ASSA 100. (Auke Slotegraaf). Messier objects. Apparent size: degrees, arc minutes, arc seconds. Interesting info. AKA’s. Emphasis, correction. Coordinates, location. Stars, star groups, etc. Variable stars. Double stars. (Only a small number included. “Colourful Ds. descriptions” taken from the book by Sissy Haas). Carbon star. C Asterisma. (Including many “Streicher” objects, taken from Asterism.
  • The Hertzsprung-Russell Diagram

    The Hertzsprung-Russell Diagram A. Luminosity, Temperature, and Size Introduction In the early part of this century, two astronomers, one Danish and one American, invented a diagram showing the basic characteristics of stars. The color-magnitude diagram, often called the Hertzsprung-Russell (HR) diagram in their honor, has proved to be the Rosetta stone of stellar astronomy. The purpose of this exercise is to give you some familiarity with the diagram. In addition, you will be asked to investigate the types of biases in measurement used to construct this diagram. Biases are especially important in understanding astronomical data. Unlike laboratory sciences, astronomical experiments must be conducted under the conditions the Universe gives us. Another way to think about this is that astronomy has no test tube! Since the astronomer has no direct control over the experiment, it is imperative that he or she understands the prejudices introduced into the data by the human perspective. However, biases of measurement are found in many other fields of science. An example of a biased study would be to find the weight vs. age relation for all Americans by weighing only members of health clubs. Most active health club members tend to be more fit than the average, and so the average derived would be lower than the true average weight of Americans. This exercise asks you to make comparisons between two different samples of stars. The bright star table was selected on the basis of apparent brightness, NOT the luminosity of the stars. The near star table is all stars within 5 parsecs (about 15-16 light years) from the Sun.
  • Stellar and Substellar Companions of Nearby Stars from Gaia DR2 Binarity from Proper Motion Anomaly?

    Stellar and Substellar Companions of Nearby Stars from Gaia DR2 Binarity from Proper Motion Anomaly?

    A&A 623, A72 (2019) Astronomy https://doi.org/10.1051/0004-6361/201834371 & c P. Kervella et al. 2019 Astrophysics Stellar and substellar companions of nearby stars from Gaia DR2 Binarity from proper motion anomaly? Pierre Kervella1, Frédéric Arenou2, François Mignard3, and Frédéric Thévenin3 1 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France e-mail: [email protected] 2 GEPI, Observatoire de Paris, Université PSL, CNRS, 5 Place Jules Janssen, 92190 Meudon, France 3 Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Lagrange UMR 7293, CS 34229, 06304 Nice Cedex 4, France Received 3 October 2018 / Accepted 26 January 2019 ABSTRACT Context. The census of stellar and substellar companions of nearby stars is largely incomplete, in particular toward the low-mass brown dwarf and long-period exoplanets. It is, however, fundamentally important in the understanding of the stellar and planetary formation and evolution mechanisms. Nearby stars are particularly favorable targets for high precision astrometry. Aims. We aim to characterize the presence of physical companions of stellar and substellar mass in orbit around nearby stars. Methods. Orbiting secondary bodies influence the proper motion of their parent star through their gravitational reflex motion. Using the Hipparcos and Gaia’s second data release (GDR2) catalogs, we determined the long-term proper motion of the stars common to these two catalogs. We then searched for a proper motion anomaly (PMa) between the long-term proper motion vector and the GDR2 (or Hipparcos) measurements, indicative of the presence of a perturbing secondary object.